Abstract A recent CO survey of the Cepheus Flare region (100°≤1≤141°, 8°≤b≤22°) has allowed a detailed study of the diffuse gamma-ray emission and the gas content of this nearby region. The comparison of the HI and CO observations with the COS-B gamma-ray data yields estimates of the N(H2)/WCO ratio in this molecular complex and of the emissivity spectrum of the gas between 70 MeV and 5 GeV. A significant (3.9σ) point-like excess above the diffuse emission has been found and can be interpreted as a new gamma-ray source.
Gamma rays and interstellar gas in the Cepheus region: A new gamma-ray source?
Advances in Space Research ; 10 , 2 ; 81-84
1989-01-01
4 pages
Article (Journal)
Electronic Resource
English
Ultrabright source produces MeV-class gamma rays
British Library Online Contents | 2008
Online Contents | 2008
|Gamma rays and the origin of cosmic rays
Elsevier | 1989
|X-Rays and Gamma Rays-Their Industrial Application
SAE Technical Papers | 1937
|Kinematic Analysis of Cepheus OB3
British Library Online Contents | 1997
|