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Molecular hydrogen in the galaxy and galactic gamma rays

Stecker, F. W. and Solomon, P. M. and Scoville, N. Z. and Ryter, C. E. (1975) Molecular hydrogen in the galaxy and galactic gamma rays. In: 14th International Cosmic Ray Conference. Vol.1. Max-Planck-Institut für Extraterrestrische Physik , Munich, pp. 46-51. https://resolver.caltech.edu/CaltechAUTHORS:20190506-144730310

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Abstract

Estimates made of column densities of H_2 at galactic longitude equals 0° indicate that H_2 is far more abundant than HI in the inner galaxy and is the key to an explanation of the gamma-ray observations. This is also reflected in the correlation of galactic longitude and latitude distributions of gamma-rays and molecular clouds. Particularly strong evidence is found from the galactic survey of CO emission at 2.64 mm. The cosmic-ray distribution inferred from the calculations is not uniform but only weakly dependent on the total gas distribution in the inner galaxy.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://adsabs.harvard.edu/abs/1975ICRC....1...46SADSArticle
http://resolver.caltech.edu/CaltechAUTHORS:20190403-153008275Related ItemJournal Article
ORCID:
AuthorORCID
Scoville, N. Z.0000-0002-0438-3323
Additional Information:© 1975 MPE. Provided by the NASA Astrophysics Data System.
Funders:
Funding AgencyGrant Number
National Research CouncilUNSPECIFIED
Record Number:CaltechAUTHORS:20190506-144730310
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190506-144730310
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:95260
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:06 May 2019 21:58
Last Modified:03 Oct 2019 21:11

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