Nucleonic gamma-ray production in pulsar wind nebulae View Full Text


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

2007-06

AUTHORS

D. Horns, F. Aharonian, A. I. D. Hoffmann, A. Santangelo

ABSTRACT

Observations of the inner radian of the Galactic disk at very high energy (VHE) gamma-rays have revealed at least 16 new sources. Besides shell type super-nova remnants, pulsar wind nebulae (PWN) appear to be a dominant source population in the catalogue of VHE gamma-ray sources. Except for the Crab nebula, the newly discovered PWN are resolved at VHE gamma-rays to be spatially extended (5–20 pc). Currently, at least 3 middle aged (t>10 kyrs) PWN (Vela X, G18.0-0.7, and G313.3+0.6 in the “Kookaburra” region) and 1 young PWN MSH 15-52 (t=1.55 kyrs) have been identified to be VHE emitting PWN (sometimes called “TeV Plerions”). Two more candidate “TeV Plerions” have been identified and have been reported at this conference (Carrigan, These proceedings, in preparation). In this contribution, the gamma-ray emission from Vela X is explained by a nucleonic component in the pulsar wind. The measured broad band spectral energy distribution is compared with the expected X-ray emission from primary and secondary electrons. The observed X-ray emission and TeV emission from the three middle aged PWN are compared with each other. More... »

PAGES

189-195

References to SciGraph publications

  • 2007-06. High energy processes in pulsar wind nebulae in ASTROPHYSICS AND SPACE SCIENCE
  • 1995-05. An X-ray jet from the Vela pulsar in NATURE
  • Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1007/s10509-007-9444-5

    DOI

    http://dx.doi.org/10.1007/s10509-007-9444-5

    DIMENSIONS

    https://app.dimensions.ai/details/publication/pub.1017149624


    Indexing Status Check whether this publication has been indexed by Scopus and Web Of Science using the SN Indexing Status Tool
    Incoming Citations Browse incoming citations for this publication using opencitations.net

    JSON-LD is the canonical representation for SciGraph data.

    TIP: You can open this SciGraph record using an external JSON-LD service: JSON-LD Playground Google SDTT

    [
      {
        "@context": "https://springernature.github.io/scigraph/jsonld/sgcontext.json", 
        "about": [
          {
            "id": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/0201", 
            "inDefinedTermSet": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/", 
            "name": "Astronomical and Space Sciences", 
            "type": "DefinedTerm"
          }, 
          {
            "id": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/02", 
            "inDefinedTermSet": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/", 
            "name": "Physical Sciences", 
            "type": "DefinedTerm"
          }
        ], 
        "author": [
          {
            "affiliation": {
              "alternateName": "University of T\u00fcbingen", 
              "id": "https://www.grid.ac/institutes/grid.10392.39", 
              "name": [
                "Institute for Astronomy and Astrophysics, Karl-Eberhards University T\u00fcbingen, Sand 1, 72076, T\u00fcbingen, Germany"
              ], 
              "type": "Organization"
            }, 
            "familyName": "Horns", 
            "givenName": "D.", 
            "id": "sg:person.011772261753.41", 
            "sameAs": [
              "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.011772261753.41"
            ], 
            "type": "Person"
          }, 
          {
            "affiliation": {
              "alternateName": "Max Planck Society", 
              "id": "https://www.grid.ac/institutes/grid.4372.2", 
              "name": [
                "Max-Planck-Institut f. Kernphysik Heidelberg, P.O. Box 10 39 80, 69117, Heidelberg, Germany"
              ], 
              "type": "Organization"
            }, 
            "familyName": "Aharonian", 
            "givenName": "F.", 
            "id": "sg:person.01354457257.24", 
            "sameAs": [
              "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.01354457257.24"
            ], 
            "type": "Person"
          }, 
          {
            "affiliation": {
              "alternateName": "University of T\u00fcbingen", 
              "id": "https://www.grid.ac/institutes/grid.10392.39", 
              "name": [
                "Institute for Astronomy and Astrophysics, Karl-Eberhards University T\u00fcbingen, Sand 1, 72076, T\u00fcbingen, Germany"
              ], 
              "type": "Organization"
            }, 
            "familyName": "Hoffmann", 
            "givenName": "A. I. D.", 
            "id": "sg:person.016550362067.17", 
            "sameAs": [
              "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.016550362067.17"
            ], 
            "type": "Person"
          }, 
          {
            "affiliation": {
              "alternateName": "University of T\u00fcbingen", 
              "id": "https://www.grid.ac/institutes/grid.10392.39", 
              "name": [
                "Institute for Astronomy and Astrophysics, Karl-Eberhards University T\u00fcbingen, Sand 1, 72076, T\u00fcbingen, Germany"
              ], 
              "type": "Organization"
            }, 
            "familyName": "Santangelo", 
            "givenName": "A.", 
            "id": "sg:person.015262403642.69", 
            "sameAs": [
              "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.015262403642.69"
            ], 
            "type": "Person"
          }
        ], 
        "citation": [
          {
            "id": "https://doi.org/10.1086/368356", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1004280241"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1093/pasj/48.2.157", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1006898345"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1111/j.1365-2966.2004.08592.x", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1010031977"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1046/j.1365-8711.2001.04851.x", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1017129743"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "sg:pub.10.1007/s10509-007-9396-9", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1023744554", 
              "https://doi.org/10.1007/s10509-007-9396-9"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "sg:pub.10.1007/s10509-007-9396-9", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1023744554", 
              "https://doi.org/10.1007/s10509-007-9396-9"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1086/500541", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1025399704"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1086/320352", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1026879605"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1103/physrevlett.80.3911", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1027641893"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1103/physrevlett.80.3911", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1027641893"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1086/323377", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1031254268"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1086/500189", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1032078739"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1086/380486", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1032138978"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1086/508050", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1032362529"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1086/430632", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1033637521"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1051/0004-6361:200600014", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1034762918"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1051/0004-6361:200600014", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1034762918"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1086/339354", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1036753744"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1046/j.1365-8711.2000.03250.x", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1037888667"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1086/376829", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1038683187"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "sg:pub.10.1038/375040a0", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1038879597", 
              "https://doi.org/10.1038/375040a0"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "sg:pub.10.1038/375040a0", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1038879597", 
              "https://doi.org/10.1038/375040a0"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1063/1.2141897", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1039489615"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1086/375531", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1041986265"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1071/ph580550", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1046641314"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1086/321533", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1046888227"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1051/0004-6361:20042367", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1056934357"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1051/0004-6361:200500180", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1056934829"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1051/0004-6361:20065116", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1056936889"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1063/1.859877", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1058113079"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1086/162356", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1058493646"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1086/171296", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1058502586"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1086/171326", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1058502616"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1086/174810", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1058506100"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1086/191832", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1058519283"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1086/310616", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1058618113"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1086/324042", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1058624365"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1086/376567", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1058669919"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1086/506322", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1058785206"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1103/physrevd.74.034018", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1060706427"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1103/physrevd.74.034018", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1060706427"
            ], 
            "type": "CreativeWork"
          }, 
          {
            "id": "https://doi.org/10.1109/23.281527", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1061129133"
            ], 
            "type": "CreativeWork"
          }
        ], 
        "datePublished": "2007-06", 
        "datePublishedReg": "2007-06-01", 
        "description": "Observations of the inner radian of the Galactic disk at very high energy (VHE) gamma-rays have revealed at least 16 new sources. Besides shell type super-nova remnants, pulsar wind nebulae (PWN) appear to be a dominant source population in the catalogue of VHE gamma-ray sources. Except for the Crab nebula, the newly discovered PWN are resolved at VHE gamma-rays to be spatially extended (5\u201320 pc). Currently, at least 3 middle aged (t>10 kyrs) PWN (Vela X, G18.0-0.7, and G313.3+0.6 in the \u201cKookaburra\u201d region) and 1 young PWN MSH 15-52 (t=1.55 kyrs) have been identified to be VHE emitting PWN (sometimes called \u201cTeV Plerions\u201d). Two more candidate \u201cTeV Plerions\u201d have been identified and have been reported at this conference (Carrigan, These proceedings, in preparation). In this contribution, the gamma-ray emission from Vela X is explained by a nucleonic component in the pulsar wind. The measured broad band spectral energy distribution is compared with the expected X-ray emission from primary and secondary electrons. The observed X-ray emission and TeV emission from the three middle aged PWN are compared with each other.", 
        "genre": "research_article", 
        "id": "sg:pub.10.1007/s10509-007-9444-5", 
        "inLanguage": [
          "en"
        ], 
        "isAccessibleForFree": true, 
        "isPartOf": [
          {
            "id": "sg:journal.1026094", 
            "issn": [
              "0004-640X", 
              "1572-946X"
            ], 
            "name": "Astrophysics and Space Science", 
            "type": "Periodical"
          }, 
          {
            "issueNumber": "1-4", 
            "type": "PublicationIssue"
          }, 
          {
            "type": "PublicationVolume", 
            "volumeNumber": "309"
          }
        ], 
        "name": "Nucleonic gamma-ray production in pulsar wind nebulae", 
        "pagination": "189-195", 
        "productId": [
          {
            "name": "readcube_id", 
            "type": "PropertyValue", 
            "value": [
              "51b5010a2cc2da4cff0097a1db4997a1987545b8e015c00f3afe5e8b1db9e0c3"
            ]
          }, 
          {
            "name": "doi", 
            "type": "PropertyValue", 
            "value": [
              "10.1007/s10509-007-9444-5"
            ]
          }, 
          {
            "name": "dimensions_id", 
            "type": "PropertyValue", 
            "value": [
              "pub.1017149624"
            ]
          }
        ], 
        "sameAs": [
          "https://doi.org/10.1007/s10509-007-9444-5", 
          "https://app.dimensions.ai/details/publication/pub.1017149624"
        ], 
        "sdDataset": "articles", 
        "sdDatePublished": "2019-04-11T12:56", 
        "sdLicense": "https://scigraph.springernature.com/explorer/license/", 
        "sdPublisher": {
          "name": "Springer Nature - SN SciGraph project", 
          "type": "Organization"
        }, 
        "sdSource": "s3://com-uberresearch-data-dimensions-target-20181106-alternative/cleanup/v134/2549eaecd7973599484d7c17b260dba0a4ecb94b/merge/v9/a6c9fde33151104705d4d7ff012ea9563521a3ce/jats-lookup/v90/0000000365_0000000365/records_71673_00000000.jsonl", 
        "type": "ScholarlyArticle", 
        "url": "http://link.springer.com/10.1007/s10509-007-9444-5"
      }
    ]
     

    Download the RDF metadata as:  json-ld nt turtle xml License info

    HOW TO GET THIS DATA PROGRAMMATICALLY:

    JSON-LD is a popular format for linked data which is fully compatible with JSON.

    curl -H 'Accept: application/ld+json' 'https://scigraph.springernature.com/pub.10.1007/s10509-007-9444-5'

    N-Triples is a line-based linked data format ideal for batch operations.

    curl -H 'Accept: application/n-triples' 'https://scigraph.springernature.com/pub.10.1007/s10509-007-9444-5'

    Turtle is a human-readable linked data format.

    curl -H 'Accept: text/turtle' 'https://scigraph.springernature.com/pub.10.1007/s10509-007-9444-5'

    RDF/XML is a standard XML format for linked data.

    curl -H 'Accept: application/rdf+xml' 'https://scigraph.springernature.com/pub.10.1007/s10509-007-9444-5'


     

    This table displays all metadata directly associated to this object as RDF triples.

    198 TRIPLES      21 PREDICATES      64 URIs      19 LITERALS      7 BLANK NODES

    Subject Predicate Object
    1 sg:pub.10.1007/s10509-007-9444-5 schema:about anzsrc-for:02
    2 anzsrc-for:0201
    3 schema:author N1d9a5397b6d14e66b48c160f876f6fcd
    4 schema:citation sg:pub.10.1007/s10509-007-9396-9
    5 sg:pub.10.1038/375040a0
    6 https://doi.org/10.1046/j.1365-8711.2000.03250.x
    7 https://doi.org/10.1046/j.1365-8711.2001.04851.x
    8 https://doi.org/10.1051/0004-6361:20042367
    9 https://doi.org/10.1051/0004-6361:200500180
    10 https://doi.org/10.1051/0004-6361:200600014
    11 https://doi.org/10.1051/0004-6361:20065116
    12 https://doi.org/10.1063/1.2141897
    13 https://doi.org/10.1063/1.859877
    14 https://doi.org/10.1071/ph580550
    15 https://doi.org/10.1086/162356
    16 https://doi.org/10.1086/171296
    17 https://doi.org/10.1086/171326
    18 https://doi.org/10.1086/174810
    19 https://doi.org/10.1086/191832
    20 https://doi.org/10.1086/310616
    21 https://doi.org/10.1086/320352
    22 https://doi.org/10.1086/321533
    23 https://doi.org/10.1086/323377
    24 https://doi.org/10.1086/324042
    25 https://doi.org/10.1086/339354
    26 https://doi.org/10.1086/368356
    27 https://doi.org/10.1086/375531
    28 https://doi.org/10.1086/376567
    29 https://doi.org/10.1086/376829
    30 https://doi.org/10.1086/380486
    31 https://doi.org/10.1086/430632
    32 https://doi.org/10.1086/500189
    33 https://doi.org/10.1086/500541
    34 https://doi.org/10.1086/506322
    35 https://doi.org/10.1086/508050
    36 https://doi.org/10.1093/pasj/48.2.157
    37 https://doi.org/10.1103/physrevd.74.034018
    38 https://doi.org/10.1103/physrevlett.80.3911
    39 https://doi.org/10.1109/23.281527
    40 https://doi.org/10.1111/j.1365-2966.2004.08592.x
    41 schema:datePublished 2007-06
    42 schema:datePublishedReg 2007-06-01
    43 schema:description Observations of the inner radian of the Galactic disk at very high energy (VHE) gamma-rays have revealed at least 16 new sources. Besides shell type super-nova remnants, pulsar wind nebulae (PWN) appear to be a dominant source population in the catalogue of VHE gamma-ray sources. Except for the Crab nebula, the newly discovered PWN are resolved at VHE gamma-rays to be spatially extended (5–20 pc). Currently, at least 3 middle aged (t>10 kyrs) PWN (Vela X, G18.0-0.7, and G313.3+0.6 in the “Kookaburra” region) and 1 young PWN MSH 15-52 (t=1.55 kyrs) have been identified to be VHE emitting PWN (sometimes called “TeV Plerions”). Two more candidate “TeV Plerions” have been identified and have been reported at this conference (Carrigan, These proceedings, in preparation). In this contribution, the gamma-ray emission from Vela X is explained by a nucleonic component in the pulsar wind. The measured broad band spectral energy distribution is compared with the expected X-ray emission from primary and secondary electrons. The observed X-ray emission and TeV emission from the three middle aged PWN are compared with each other.
    44 schema:genre research_article
    45 schema:inLanguage en
    46 schema:isAccessibleForFree true
    47 schema:isPartOf N1d5873bac1de48a0adeeca9538441aa6
    48 N68072597310f471ab11f66eb5a4a32b6
    49 sg:journal.1026094
    50 schema:name Nucleonic gamma-ray production in pulsar wind nebulae
    51 schema:pagination 189-195
    52 schema:productId N0b3591a8c316470099d0927bb1cd0944
    53 N97bbbd8e2872404998ea9e4a5fc0129d
    54 Nd051369f9e5240a5a498933d449c4d97
    55 schema:sameAs https://app.dimensions.ai/details/publication/pub.1017149624
    56 https://doi.org/10.1007/s10509-007-9444-5
    57 schema:sdDatePublished 2019-04-11T12:56
    58 schema:sdLicense https://scigraph.springernature.com/explorer/license/
    59 schema:sdPublisher N023fffef10134cf28a715195279d38b8
    60 schema:url http://link.springer.com/10.1007/s10509-007-9444-5
    61 sgo:license sg:explorer/license/
    62 sgo:sdDataset articles
    63 rdf:type schema:ScholarlyArticle
    64 N023fffef10134cf28a715195279d38b8 schema:name Springer Nature - SN SciGraph project
    65 rdf:type schema:Organization
    66 N0b3591a8c316470099d0927bb1cd0944 schema:name dimensions_id
    67 schema:value pub.1017149624
    68 rdf:type schema:PropertyValue
    69 N15314b8809324af7ba6e2c3ac5bc7fb9 rdf:first sg:person.016550362067.17
    70 rdf:rest N7a9fb4279b0c45ceaf9a673e243e409c
    71 N1d5873bac1de48a0adeeca9538441aa6 schema:issueNumber 1-4
    72 rdf:type schema:PublicationIssue
    73 N1d9a5397b6d14e66b48c160f876f6fcd rdf:first sg:person.011772261753.41
    74 rdf:rest N43439c925da0441baf98add600a8e8cb
    75 N43439c925da0441baf98add600a8e8cb rdf:first sg:person.01354457257.24
    76 rdf:rest N15314b8809324af7ba6e2c3ac5bc7fb9
    77 N68072597310f471ab11f66eb5a4a32b6 schema:volumeNumber 309
    78 rdf:type schema:PublicationVolume
    79 N7a9fb4279b0c45ceaf9a673e243e409c rdf:first sg:person.015262403642.69
    80 rdf:rest rdf:nil
    81 N97bbbd8e2872404998ea9e4a5fc0129d schema:name readcube_id
    82 schema:value 51b5010a2cc2da4cff0097a1db4997a1987545b8e015c00f3afe5e8b1db9e0c3
    83 rdf:type schema:PropertyValue
    84 Nd051369f9e5240a5a498933d449c4d97 schema:name doi
    85 schema:value 10.1007/s10509-007-9444-5
    86 rdf:type schema:PropertyValue
    87 anzsrc-for:02 schema:inDefinedTermSet anzsrc-for:
    88 schema:name Physical Sciences
    89 rdf:type schema:DefinedTerm
    90 anzsrc-for:0201 schema:inDefinedTermSet anzsrc-for:
    91 schema:name Astronomical and Space Sciences
    92 rdf:type schema:DefinedTerm
    93 sg:journal.1026094 schema:issn 0004-640X
    94 1572-946X
    95 schema:name Astrophysics and Space Science
    96 rdf:type schema:Periodical
    97 sg:person.011772261753.41 schema:affiliation https://www.grid.ac/institutes/grid.10392.39
    98 schema:familyName Horns
    99 schema:givenName D.
    100 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.011772261753.41
    101 rdf:type schema:Person
    102 sg:person.01354457257.24 schema:affiliation https://www.grid.ac/institutes/grid.4372.2
    103 schema:familyName Aharonian
    104 schema:givenName F.
    105 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.01354457257.24
    106 rdf:type schema:Person
    107 sg:person.015262403642.69 schema:affiliation https://www.grid.ac/institutes/grid.10392.39
    108 schema:familyName Santangelo
    109 schema:givenName A.
    110 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.015262403642.69
    111 rdf:type schema:Person
    112 sg:person.016550362067.17 schema:affiliation https://www.grid.ac/institutes/grid.10392.39
    113 schema:familyName Hoffmann
    114 schema:givenName A. I. D.
    115 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.016550362067.17
    116 rdf:type schema:Person
    117 sg:pub.10.1007/s10509-007-9396-9 schema:sameAs https://app.dimensions.ai/details/publication/pub.1023744554
    118 https://doi.org/10.1007/s10509-007-9396-9
    119 rdf:type schema:CreativeWork
    120 sg:pub.10.1038/375040a0 schema:sameAs https://app.dimensions.ai/details/publication/pub.1038879597
    121 https://doi.org/10.1038/375040a0
    122 rdf:type schema:CreativeWork
    123 https://doi.org/10.1046/j.1365-8711.2000.03250.x schema:sameAs https://app.dimensions.ai/details/publication/pub.1037888667
    124 rdf:type schema:CreativeWork
    125 https://doi.org/10.1046/j.1365-8711.2001.04851.x schema:sameAs https://app.dimensions.ai/details/publication/pub.1017129743
    126 rdf:type schema:CreativeWork
    127 https://doi.org/10.1051/0004-6361:20042367 schema:sameAs https://app.dimensions.ai/details/publication/pub.1056934357
    128 rdf:type schema:CreativeWork
    129 https://doi.org/10.1051/0004-6361:200500180 schema:sameAs https://app.dimensions.ai/details/publication/pub.1056934829
    130 rdf:type schema:CreativeWork
    131 https://doi.org/10.1051/0004-6361:200600014 schema:sameAs https://app.dimensions.ai/details/publication/pub.1034762918
    132 rdf:type schema:CreativeWork
    133 https://doi.org/10.1051/0004-6361:20065116 schema:sameAs https://app.dimensions.ai/details/publication/pub.1056936889
    134 rdf:type schema:CreativeWork
    135 https://doi.org/10.1063/1.2141897 schema:sameAs https://app.dimensions.ai/details/publication/pub.1039489615
    136 rdf:type schema:CreativeWork
    137 https://doi.org/10.1063/1.859877 schema:sameAs https://app.dimensions.ai/details/publication/pub.1058113079
    138 rdf:type schema:CreativeWork
    139 https://doi.org/10.1071/ph580550 schema:sameAs https://app.dimensions.ai/details/publication/pub.1046641314
    140 rdf:type schema:CreativeWork
    141 https://doi.org/10.1086/162356 schema:sameAs https://app.dimensions.ai/details/publication/pub.1058493646
    142 rdf:type schema:CreativeWork
    143 https://doi.org/10.1086/171296 schema:sameAs https://app.dimensions.ai/details/publication/pub.1058502586
    144 rdf:type schema:CreativeWork
    145 https://doi.org/10.1086/171326 schema:sameAs https://app.dimensions.ai/details/publication/pub.1058502616
    146 rdf:type schema:CreativeWork
    147 https://doi.org/10.1086/174810 schema:sameAs https://app.dimensions.ai/details/publication/pub.1058506100
    148 rdf:type schema:CreativeWork
    149 https://doi.org/10.1086/191832 schema:sameAs https://app.dimensions.ai/details/publication/pub.1058519283
    150 rdf:type schema:CreativeWork
    151 https://doi.org/10.1086/310616 schema:sameAs https://app.dimensions.ai/details/publication/pub.1058618113
    152 rdf:type schema:CreativeWork
    153 https://doi.org/10.1086/320352 schema:sameAs https://app.dimensions.ai/details/publication/pub.1026879605
    154 rdf:type schema:CreativeWork
    155 https://doi.org/10.1086/321533 schema:sameAs https://app.dimensions.ai/details/publication/pub.1046888227
    156 rdf:type schema:CreativeWork
    157 https://doi.org/10.1086/323377 schema:sameAs https://app.dimensions.ai/details/publication/pub.1031254268
    158 rdf:type schema:CreativeWork
    159 https://doi.org/10.1086/324042 schema:sameAs https://app.dimensions.ai/details/publication/pub.1058624365
    160 rdf:type schema:CreativeWork
    161 https://doi.org/10.1086/339354 schema:sameAs https://app.dimensions.ai/details/publication/pub.1036753744
    162 rdf:type schema:CreativeWork
    163 https://doi.org/10.1086/368356 schema:sameAs https://app.dimensions.ai/details/publication/pub.1004280241
    164 rdf:type schema:CreativeWork
    165 https://doi.org/10.1086/375531 schema:sameAs https://app.dimensions.ai/details/publication/pub.1041986265
    166 rdf:type schema:CreativeWork
    167 https://doi.org/10.1086/376567 schema:sameAs https://app.dimensions.ai/details/publication/pub.1058669919
    168 rdf:type schema:CreativeWork
    169 https://doi.org/10.1086/376829 schema:sameAs https://app.dimensions.ai/details/publication/pub.1038683187
    170 rdf:type schema:CreativeWork
    171 https://doi.org/10.1086/380486 schema:sameAs https://app.dimensions.ai/details/publication/pub.1032138978
    172 rdf:type schema:CreativeWork
    173 https://doi.org/10.1086/430632 schema:sameAs https://app.dimensions.ai/details/publication/pub.1033637521
    174 rdf:type schema:CreativeWork
    175 https://doi.org/10.1086/500189 schema:sameAs https://app.dimensions.ai/details/publication/pub.1032078739
    176 rdf:type schema:CreativeWork
    177 https://doi.org/10.1086/500541 schema:sameAs https://app.dimensions.ai/details/publication/pub.1025399704
    178 rdf:type schema:CreativeWork
    179 https://doi.org/10.1086/506322 schema:sameAs https://app.dimensions.ai/details/publication/pub.1058785206
    180 rdf:type schema:CreativeWork
    181 https://doi.org/10.1086/508050 schema:sameAs https://app.dimensions.ai/details/publication/pub.1032362529
    182 rdf:type schema:CreativeWork
    183 https://doi.org/10.1093/pasj/48.2.157 schema:sameAs https://app.dimensions.ai/details/publication/pub.1006898345
    184 rdf:type schema:CreativeWork
    185 https://doi.org/10.1103/physrevd.74.034018 schema:sameAs https://app.dimensions.ai/details/publication/pub.1060706427
    186 rdf:type schema:CreativeWork
    187 https://doi.org/10.1103/physrevlett.80.3911 schema:sameAs https://app.dimensions.ai/details/publication/pub.1027641893
    188 rdf:type schema:CreativeWork
    189 https://doi.org/10.1109/23.281527 schema:sameAs https://app.dimensions.ai/details/publication/pub.1061129133
    190 rdf:type schema:CreativeWork
    191 https://doi.org/10.1111/j.1365-2966.2004.08592.x schema:sameAs https://app.dimensions.ai/details/publication/pub.1010031977
    192 rdf:type schema:CreativeWork
    193 https://www.grid.ac/institutes/grid.10392.39 schema:alternateName University of Tübingen
    194 schema:name Institute for Astronomy and Astrophysics, Karl-Eberhards University Tübingen, Sand 1, 72076, Tübingen, Germany
    195 rdf:type schema:Organization
    196 https://www.grid.ac/institutes/grid.4372.2 schema:alternateName Max Planck Society
    197 schema:name Max-Planck-Institut f. Kernphysik Heidelberg, P.O. Box 10 39 80, 69117, Heidelberg, Germany
    198 rdf:type schema:Organization
     




    Preview window. Press ESC to close (or click here)


    ...