Brackett-γ Line Survey of the Ionized Hydrogen in the Galactic Plane View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

2005

AUTHORS

A. S. Kutyrev , C. L. Bennett , S. H. Moseley , R. J. Reynolds , F. L. Roesler

ABSTRACT

We have carried out a 2.1655 micron Brackett-gamma hydrogen recombination emission line pilot survey of the Galactic plane using a Goddard-Wisconsin cryogenic Fabry-Perot spectrometer. For this survey fields were selected along the Galactic plane from 358° to 43° longitude. The velocity range of the observed emission features ranges from −10 km s−1 to 90 km s−1 (LSR). Typical detected intensities correspond to emission measures of about 1000 cm−6 pc. More... »

PAGES

79-82

Book

TITLE

How does the Galaxy Work?

ISBN

1-4020-2619-6

Author Affiliations

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/1-4020-2620-x_14

DOI

http://dx.doi.org/10.1007/1-4020-2620-x_14

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1000068538


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