Publication Abstracts
Arnaud et al. 1982
Arnaud, K., L.T. Pei, P.A. Riley, A.W. Wolfendale, T.M. Dame, J.E. Brock, and P. Thaddeus, 1982: The interrelation of cosmic γ-rays and interstellar gas in the range l:65-180°. Mon. Not. Roy. Astron. Soc., 201, 745-758.
New date on the distribution of molecular hydrogen in the first and second quadrants allow a detailed analysis of the relationship between the column density of gas (in all major forms) and the intensity of cosmic γ-rays in the Galaxy.
It is concluded that most of the features observed in the gamma-ray map can be explained in terms of cosmic-ray interactions with the gas in the ISM, with molecular hydrogen playing an important role. The cosmic-ray intensity in the important production regions appears to be roughly independent of galactocentric distance, R, for l:65-100°d to fall off slowly with R for l:100-180°.
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BibTeX Citation
@article{ar01100t,
author={Arnaud, K. and Pei, L. T. and Riley, P. A. and Wolfendale, A. W. and Dame, T. M. and Brock, J. E. and Thaddeus, P.},
title={The interrelation of cosmic γ-rays and interstellar gas in the range l:65-180°},
year={1982},
journal={Monthly Notices of the Royal Astronomical Society},
volume={201},
pages={745--758},
}
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RIS Citation
TY - JOUR ID - ar01100t AU - Arnaud, K. AU - Pei, L. T. AU - Riley, P. A. AU - Wolfendale, A. W. AU - Dame, T. M. AU - Brock, J. E. AU - Thaddeus, P. PY - 1982 TI - The interrelation of cosmic γ-rays and interstellar gas in the range l:65-180° JA - Mon. Not. Roy. Astron. Soc. JO - Monthly Notices of the Royal Astronomical Society VL - 201 SP - 745 EP - 758 ER -
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