Galactic gamma-ray sources, SNOBs, and giant H2 regions

Details Galactic gamma-ray sources, SNOBs, and giant H2 regions Galactic gamma-ray sources, SNOBs, and giant H2 regions

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....1..209m&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 1 p 209-212 (SEE N85-33902 22-93)

Other

Galactic Radiation, Molecular Clouds, Radiation Sources, Variable Stars, Carbon Monoxide, Cos-B Satellite, Pulsars, Spiral Galaxies, Wavelengths

Scientific paper

Progress towards understanding the nature of the COS-B galactic gamma-ray sources was made by two recent developments. The developments are: (1) the existence of extensive wide-latitude CO surveys, from the Northern Hemisphere, and from the Southern Hemisphere which give more precise information on molecular cloud population of the Perseus, Sagittarius, and Carina spiral arms; (2) the study of the time variability of gamma-ray sources in gamma-rays but also at other wavelengths, leading to the discovery of four new variable sources in addition to the already known Crab and Vela pulsars. Three classes of gamma-ray sources are found; invariable sources, active sources, and passive sources.

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