Problems of star-formation theory and prospects for submillimeter observations View Full Text


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

2008-11-28

AUTHORS

D. Z. Wiebe, M. S. Kirsanova, B. M. Shustov, Ya. N. Pavlyuchenkov

ABSTRACT

We consider the current state of star-formation theory and requirements for millimeter and submillimeter observations that would enable the resolution of the most pressing problems in the physics of star formation. Two key features of star-forming regions that define these observational requirements are the relatively low energy of processes taking place there and the smallness of the corresponding spatial scales. This is especially true for objects in the latest stages of “pre-stellar” evolution, that is, hot cores, hypercompact and ultracompact HII regions, and protoplanetary disks. The angular resolution, sensitivity, and spectral coverage in existing ground-based and space submillimeter and millimeter telescopes are not fully adequate to the observtional requirements. To obtain detailed information on star-forming regions, as well as individual protostars, it is necessary to use a space-based interferometer. More... »

PAGES

976-984

Identifiers

URI

http://scigraph.springernature.com/pub.10.1134/s1063772908120032

DOI

http://dx.doi.org/10.1134/s1063772908120032

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1049330643


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/2008/02", 
        "inDefinedTermSet": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/", 
        "name": "Physical Sciences", 
        "type": "DefinedTerm"
      }, 
      {
        "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"
      }
    ], 
    "author": [
      {
        "affiliation": {
          "alternateName": "Institute of Astronomy, Russian Academy of Sciences, Moscow, Russia", 
          "id": "http://www.grid.ac/institutes/grid.465335.2", 
          "name": [
            "Institute of Astronomy, Russian Academy of Sciences, Moscow, Russia"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Wiebe", 
        "givenName": "D. Z.", 
        "id": "sg:person.013201612607.52", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.013201612607.52"
        ], 
        "type": "Person"
      }, 
      {
        "affiliation": {
          "alternateName": "Institute of Astronomy, Russian Academy of Sciences, Moscow, Russia", 
          "id": "http://www.grid.ac/institutes/grid.465335.2", 
          "name": [
            "Institute of Astronomy, Russian Academy of Sciences, Moscow, Russia"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Kirsanova", 
        "givenName": "M. S.", 
        "id": "sg:person.013607324544.42", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.013607324544.42"
        ], 
        "type": "Person"
      }, 
      {
        "affiliation": {
          "alternateName": "Institute of Astronomy, Russian Academy of Sciences, Moscow, Russia", 
          "id": "http://www.grid.ac/institutes/grid.465335.2", 
          "name": [
            "Institute of Astronomy, Russian Academy of Sciences, Moscow, Russia"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Shustov", 
        "givenName": "B. M.", 
        "id": "sg:person.015263656657.79", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.015263656657.79"
        ], 
        "type": "Person"
      }, 
      {
        "affiliation": {
          "alternateName": "Institute of Astronomy, Russian Academy of Sciences, Moscow, Russia", 
          "id": "http://www.grid.ac/institutes/grid.465335.2", 
          "name": [
            "Institute of Astronomy, Russian Academy of Sciences, Moscow, Russia"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Pavlyuchenkov", 
        "givenName": "Ya. N.", 
        "id": "sg:person.012666170751.33", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.012666170751.33"
        ], 
        "type": "Person"
      }
    ], 
    "datePublished": "2008-11-28", 
    "datePublishedReg": "2008-11-28", 
    "description": "We consider the current state of star-formation theory and requirements for millimeter and submillimeter observations that would enable the resolution of the most pressing problems in the physics of star formation. Two key features of star-forming regions that define these observational requirements are the relatively low energy of processes taking place there and the smallness of the corresponding spatial scales. This is especially true for objects in the latest stages of \u201cpre-stellar\u201d evolution, that is, hot cores, hypercompact and ultracompact HII regions, and protoplanetary disks. The angular resolution, sensitivity, and spectral coverage in existing ground-based and space submillimeter and millimeter telescopes are not fully adequate to the observtional requirements. To obtain detailed information on star-forming regions, as well as individual protostars, it is necessary to use a space-based interferometer.", 
    "genre": "article", 
    "id": "sg:pub.10.1134/s1063772908120032", 
    "inLanguage": "en", 
    "isAccessibleForFree": true, 
    "isPartOf": [
      {
        "id": "sg:journal.1136138", 
        "issn": [
          "0004-6299", 
          "1063-7729"
        ], 
        "name": "Astronomy Reports", 
        "publisher": "Pleiades Publishing", 
        "type": "Periodical"
      }, 
      {
        "issueNumber": "12", 
        "type": "PublicationIssue"
      }, 
      {
        "type": "PublicationVolume", 
        "volumeNumber": "52"
      }
    ], 
    "keywords": [
      "star formation theories", 
      "star-forming regions", 
      "submillimeter observations", 
      "space-based interferometers", 
      "ultracompact HII regions", 
      "star formation", 
      "individual protostars", 
      "HII regions", 
      "Millimeter Telescope", 
      "protoplanetary disks", 
      "spectral coverage", 
      "angular resolution", 
      "low energy", 
      "hot core", 
      "observational requirements", 
      "telescope", 
      "protostars", 
      "interferometer", 
      "submillimeter", 
      "physics", 
      "resolution", 
      "energy", 
      "smallness", 
      "theory", 
      "disk", 
      "millimeters", 
      "detailed information", 
      "region", 
      "state", 
      "spatial scales", 
      "objects", 
      "evolution", 
      "core", 
      "prospects", 
      "formation", 
      "key features", 
      "sensitivity", 
      "scale", 
      "current state", 
      "features", 
      "coverage", 
      "process", 
      "requirements", 
      "pressing problems", 
      "information", 
      "place", 
      "problem", 
      "later stages", 
      "stage", 
      "observations"
    ], 
    "name": "Problems of star-formation theory and prospects for submillimeter observations", 
    "pagination": "976-984", 
    "productId": [
      {
        "name": "dimensions_id", 
        "type": "PropertyValue", 
        "value": [
          "pub.1049330643"
        ]
      }, 
      {
        "name": "doi", 
        "type": "PropertyValue", 
        "value": [
          "10.1134/s1063772908120032"
        ]
      }
    ], 
    "sameAs": [
      "https://doi.org/10.1134/s1063772908120032", 
      "https://app.dimensions.ai/details/publication/pub.1049330643"
    ], 
    "sdDataset": "articles", 
    "sdDatePublished": "2022-06-01T22:08", 
    "sdLicense": "https://scigraph.springernature.com/explorer/license/", 
    "sdPublisher": {
      "name": "Springer Nature - SN SciGraph project", 
      "type": "Organization"
    }, 
    "sdSource": "s3://com-springernature-scigraph/baseset/20220601/entities/gbq_results/article/article_456.jsonl", 
    "type": "ScholarlyArticle", 
    "url": "https://doi.org/10.1134/s1063772908120032"
  }
]
 

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.10.1134/s1063772908120032'

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

curl -H 'Accept: application/n-triples' 'https://scigraph.springernature.com/pub.10.1134/s1063772908120032'

Turtle is a human-readable linked data format.

curl -H 'Accept: text/turtle' 'https://scigraph.springernature.com/pub.10.1134/s1063772908120032'

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

curl -H 'Accept: application/rdf+xml' 'https://scigraph.springernature.com/pub.10.1134/s1063772908120032'


 

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

129 TRIPLES      21 PREDICATES      75 URIs      67 LITERALS      6 BLANK NODES

Subject Predicate Object
1 sg:pub.10.1134/s1063772908120032 schema:about anzsrc-for:02
2 anzsrc-for:0201
3 schema:author Nf75869cc8171452ab7af40848047dc13
4 schema:datePublished 2008-11-28
5 schema:datePublishedReg 2008-11-28
6 schema:description We consider the current state of star-formation theory and requirements for millimeter and submillimeter observations that would enable the resolution of the most pressing problems in the physics of star formation. Two key features of star-forming regions that define these observational requirements are the relatively low energy of processes taking place there and the smallness of the corresponding spatial scales. This is especially true for objects in the latest stages of “pre-stellar” evolution, that is, hot cores, hypercompact and ultracompact HII regions, and protoplanetary disks. The angular resolution, sensitivity, and spectral coverage in existing ground-based and space submillimeter and millimeter telescopes are not fully adequate to the observtional requirements. To obtain detailed information on star-forming regions, as well as individual protostars, it is necessary to use a space-based interferometer.
7 schema:genre article
8 schema:inLanguage en
9 schema:isAccessibleForFree true
10 schema:isPartOf N1ad2f79fd2eb411fa2e69ad5d45f7715
11 Nfe715efa95c747de818ab5cbb34bb6b8
12 sg:journal.1136138
13 schema:keywords HII regions
14 Millimeter Telescope
15 angular resolution
16 core
17 coverage
18 current state
19 detailed information
20 disk
21 energy
22 evolution
23 features
24 formation
25 hot core
26 individual protostars
27 information
28 interferometer
29 key features
30 later stages
31 low energy
32 millimeters
33 objects
34 observational requirements
35 observations
36 physics
37 place
38 pressing problems
39 problem
40 process
41 prospects
42 protoplanetary disks
43 protostars
44 region
45 requirements
46 resolution
47 scale
48 sensitivity
49 smallness
50 space-based interferometers
51 spatial scales
52 spectral coverage
53 stage
54 star formation
55 star formation theories
56 star-forming regions
57 state
58 submillimeter
59 submillimeter observations
60 telescope
61 theory
62 ultracompact HII regions
63 schema:name Problems of star-formation theory and prospects for submillimeter observations
64 schema:pagination 976-984
65 schema:productId N027950a3600c48f7959624932696df0d
66 Ne0e7765e71fa46f1bd19d1c6725925f7
67 schema:sameAs https://app.dimensions.ai/details/publication/pub.1049330643
68 https://doi.org/10.1134/s1063772908120032
69 schema:sdDatePublished 2022-06-01T22:08
70 schema:sdLicense https://scigraph.springernature.com/explorer/license/
71 schema:sdPublisher N6d8b891be90a4555b2d9e763d43fc378
72 schema:url https://doi.org/10.1134/s1063772908120032
73 sgo:license sg:explorer/license/
74 sgo:sdDataset articles
75 rdf:type schema:ScholarlyArticle
76 N027950a3600c48f7959624932696df0d schema:name dimensions_id
77 schema:value pub.1049330643
78 rdf:type schema:PropertyValue
79 N1ad2f79fd2eb411fa2e69ad5d45f7715 schema:issueNumber 12
80 rdf:type schema:PublicationIssue
81 N418b580079ae47c797792bdbec1dc4fa rdf:first sg:person.012666170751.33
82 rdf:rest rdf:nil
83 N6d8b891be90a4555b2d9e763d43fc378 schema:name Springer Nature - SN SciGraph project
84 rdf:type schema:Organization
85 N814a71c36bb74b0c8fe3c79c363e8154 rdf:first sg:person.013607324544.42
86 rdf:rest N93599c533a1540cc8be3c97825d937eb
87 N93599c533a1540cc8be3c97825d937eb rdf:first sg:person.015263656657.79
88 rdf:rest N418b580079ae47c797792bdbec1dc4fa
89 Ne0e7765e71fa46f1bd19d1c6725925f7 schema:name doi
90 schema:value 10.1134/s1063772908120032
91 rdf:type schema:PropertyValue
92 Nf75869cc8171452ab7af40848047dc13 rdf:first sg:person.013201612607.52
93 rdf:rest N814a71c36bb74b0c8fe3c79c363e8154
94 Nfe715efa95c747de818ab5cbb34bb6b8 schema:volumeNumber 52
95 rdf:type schema:PublicationVolume
96 anzsrc-for:02 schema:inDefinedTermSet anzsrc-for:
97 schema:name Physical Sciences
98 rdf:type schema:DefinedTerm
99 anzsrc-for:0201 schema:inDefinedTermSet anzsrc-for:
100 schema:name Astronomical and Space Sciences
101 rdf:type schema:DefinedTerm
102 sg:journal.1136138 schema:issn 0004-6299
103 1063-7729
104 schema:name Astronomy Reports
105 schema:publisher Pleiades Publishing
106 rdf:type schema:Periodical
107 sg:person.012666170751.33 schema:affiliation grid-institutes:grid.465335.2
108 schema:familyName Pavlyuchenkov
109 schema:givenName Ya. N.
110 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.012666170751.33
111 rdf:type schema:Person
112 sg:person.013201612607.52 schema:affiliation grid-institutes:grid.465335.2
113 schema:familyName Wiebe
114 schema:givenName D. Z.
115 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.013201612607.52
116 rdf:type schema:Person
117 sg:person.013607324544.42 schema:affiliation grid-institutes:grid.465335.2
118 schema:familyName Kirsanova
119 schema:givenName M. S.
120 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.013607324544.42
121 rdf:type schema:Person
122 sg:person.015263656657.79 schema:affiliation grid-institutes:grid.465335.2
123 schema:familyName Shustov
124 schema:givenName B. M.
125 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.015263656657.79
126 rdf:type schema:Person
127 grid-institutes:grid.465335.2 schema:alternateName Institute of Astronomy, Russian Academy of Sciences, Moscow, Russia
128 schema:name Institute of Astronomy, Russian Academy of Sciences, Moscow, Russia
129 rdf:type schema:Organization
 




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


...