Hostname: page-component-cd9895bd7-jkksz Total loading time: 0 Render date: 2024-12-26T03:43:06.253Z Has data issue: false hasContentIssue false
  • English
  • Français

The high-latitude distribution of Galactic gamma rays and possible evidence for a gamma-ray halo

Published online by Cambridge University Press:  04 August 2017

A. W. Strong
A. W. Strong*
Affiliation:
Istituto di Fisica Cosmica del CNR, Milano, Italy (on behalf of the Caravane Collaboration)

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

During its 6.7-year lifetime the COS-B experiment included about 15 months of observations towards latitudes |b|> 20° and covered almost all latitudes from the South to North galactic poles. Studies comparing the local gamma-ray emission with the distribution of gas (Lebrun et al. 1982, Strong et al. 1982) have so far been limited to 10°<|b|< 20°, where the correlation is found to be fairly good and the structured emission can therefore be attributed mainly to cosmic-ray interactions with gas. The extension of this type of analysis to higher latitudes is now possible using the COS-B database.

Type
PART II: COMPOSITION, STRUCTURE AND KINEMATICS
Information
Symposium - International Astronomical Union , Volume 106: The Milky Way Galaxy , 1985 , pp. 235 - 236
Copyright
Copyright © Reidel 1985 

References

Fichtel, C.E. et al.: 1978, NASA Technical Memorandum No. 79650 Google Scholar
Iwan, D. et al.: 1982, Astrophys. J. 260, 111 CrossRefGoogle Scholar
Lebrun, F. et al.: 1982, Astron. Astrophys. 107, 390 Google Scholar
Protheroe, R.J. et al.: 1980, M.N.R.A.S. 192, 445 CrossRefGoogle Scholar
Strong, A.W. et al.: 1982, Astron. Astrophys. 115, 404 Google Scholar
Thompson, D.A., and Fichtel, C.E.: 1982, Astrophys. J. 109, 352 Google Scholar
Warwick, R.S. et al.: 1980, M.N.R.A.S. 190, 243 CrossRefGoogle Scholar
Worrall, D.M., and Strong, A.W.: 1977, Astron. Astrophys. 57, 229 Google Scholar