Local theories of the x-ray background
Conference
·
· Int. Astron. Union Symp., no. 55, pp. 258-275
OSTI ID:4426189
From symposium X - and gamma -ray astronomy; Madrid, Spain (11 May 1972). See CONF-720599-. Recent theories of the origins of diffuse-background x rays are reviewed, with emphasis on theories of the soft flux in the galactic plane and at the poles. This is probably partly galactic and partly extragalactic in origin. Failure to observe absorption by the Small Magellanic Cloud and by galactic gas in neighboring directions may be due to sources in the Cloud and to statistical fluctuations in galactic emission and absorption. Several models for numerous low-luminosity sources in the Galaxy are available. True diffuse'' emission seems unnecessary. Absorption by galactic gas seems to agree roughly with theory. The soft extragalactic component may arise in a hot intergalactic medium. The existence of a diffuse'' galactic-plane excess in 1 to 100 keV is in some doubt. Low-luminosity sources may contribute to this as well. For isotropic x-rays in 1 keV to 1 MeV, superposition theories involving clusters of galaxies, Seyfert galaxies, etc. over a cosmological path length are now roughly viable. Simple metagalactic'' Compton theories seem excluded if the break at 40 keV is sharp, but this is now in doubt. A very hot intergalactic medium at T approximately 3 x 10/sup 8/ K would give the possibility of a sharp break. A recent upper limit on the line source strength of 100-MeV photons in the galactic plane may create some difficulties for cosmic-ray theory. The spectral shape of pi -- gamma photons has become a matter of theoretical dispute. (auth)
- Research Organization:
- Univ. of Arizona, Tucson
- NSA Number:
- NSA-29-008554
- OSTI ID:
- 4426189
- Conference Information:
- Journal Name: Int. Astron. Union Symp., no. 55, pp. 258-275
- Country of Publication:
- Country unknown/Code not available
- Language:
- English
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