SIGNATURE OF A PULSAR ON THE DIFFUSE X-RAY BACKGROUND.
Journal Article
·
· Astrophys. J. 166: No. 2, L39-44(1 Jun 1971).
- Research Organization:
- Univ. of California, Berkeley
- Sponsoring Organization:
- USDOE
- NSA Number:
- NSA-25-033042
- OSTI ID:
- 4048467
- Journal Information:
- Astrophys. J. 166: No. 2, L39-44(1 Jun 1971)., Other Information: Orig. Receipt Date: 31-DEC-71
- Country of Publication:
- Country unknown/Code not available
- Language:
- English
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Related Subjects
N32170* -Physics-Astrophysics-Cosmology
N32130 - Physics-Astrophysics-Quasi-stellar
Radio & X-Ray Sources
BACKGROUND
EMISSION
KEV RANGE 01-10
PULSARS
SPECTRA
X RADIATION
X RADIATION/spectra of cosmic background
line feature at 6 to 8 keV due to young pulsars
(T)
PULSARS/x-ray emission by young
effects on diffuse background
(T)
N32130 - Physics-Astrophysics-Quasi-stellar
Radio & X-Ray Sources
BACKGROUND
EMISSION
KEV RANGE 01-10
PULSARS
SPECTRA
X RADIATION
X RADIATION/spectra of cosmic background
line feature at 6 to 8 keV due to young pulsars
(T)
PULSARS/x-ray emission by young
effects on diffuse background
(T)