COMMENT ON INVERSE COMPTON MODELS FOR THE ISOTROPIC X-RAY BACKGROUND AND POSSIBLE THERMAL EMISSION FROM A HOT INTERGALACTIC GAS.
Journal Article
·
· Astrophys. J. 177: No. 3, 585-93(1 Nov 1972).
- Research Organization:
- Univ. of California, Berkeley
- Sponsoring Organization:
- USDOE
- NSA Number:
- NSA-27-005936
- OSTI ID:
- 4587413
- Journal Information:
- Astrophys. J. 177: No. 3, 585-93(1 Nov 1972)., Other Information: Orig. Receipt Date: 30-JUN-73
- Country of Publication:
- Country unknown/Code not available
- Language:
- English
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Related Subjects
N56600* -Physics (Astrophysics & Cosmology)-Cosmology
BACKGROUND RADIATION
ELECTRONS
EMISSION
ISOTROPY
MICROWAVE RADIATION
RELATIVISTIC RANGE
SCATTERING
SPECTRA
THERMAL RADIATION
X RADIATION
MICROWAVES/cosmic background
Compton scattering by relativistic electrons
(T)
X RADIATION/cosmic background
spectrum from inverse Compton models for isotropic
(T)
ELECTRONS/scattering of cosmic background photons on relativistic
(T)
BACKGROUND RADIATION
ELECTRONS
EMISSION
ISOTROPY
MICROWAVE RADIATION
RELATIVISTIC RANGE
SCATTERING
SPECTRA
THERMAL RADIATION
X RADIATION
MICROWAVES/cosmic background
Compton scattering by relativistic electrons
(T)
X RADIATION/cosmic background
spectrum from inverse Compton models for isotropic
(T)
ELECTRONS/scattering of cosmic background photons on relativistic
(T)