Radio emission from the x-ray source A0620--00
Journal Article
·
· Astrophys. J., Lett., v. 203, no. 1, pp. L15-L16
Observations are reported of radio emission from the transient X-ray source A0620-00. Data obtained over the period 1975 August 15 to August 22 at frequencies between 1400 and 2695 MHz indicate a decaying radio event. The radio event appears to be quite different from those associated with recent galactic novae and is difficult to reconcile with a standard thermal model. A nonthermal event similar to those associated with Cygnus X-3, however, is consistent with the observations. (AIP)
- Research Organization:
- National Radio Astronomy Observatory, Green Bank, West Virginia
- Sponsoring Organization:
- USDOE
- NSA Number:
- NSA-33-027025
- OSTI ID:
- 4008171
- Journal Information:
- Astrophys. J., Lett., v. 203, no. 1, pp. L15-L16, Journal Name: Astrophys. J., Lett., v. 203, no. 1, pp. L15-L16; ISSN AJLEA
- Country of Publication:
- United States
- Language:
- English
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OSTI ID:4004081
X-ray Nova A0620--00: Celestial position and low-energy flux
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·
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Search for X-ray line emission from A0620--00
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· Astrophys. J., Lett.; (United States)
·
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Related Subjects
*COSMIC X-RAY SOURCES-- RADIOWAVE RADIATION
*NOVAE-- RADIANT FLUX DENSITY
640103* --Physics Research--Astrophysics & Cosmology--Quasi- Stellar
Radio & X-Ray Sources
EMISSION
FREQUENCY DEPENDENCE
HEATING
N56300* --Physics (Astrophysics & Cosmology)--Quasi-stellar
Radio & X-Ray Sources
SYNCHROTRON RADIATION
*NOVAE-- RADIANT FLUX DENSITY
640103* --Physics Research--Astrophysics & Cosmology--Quasi- Stellar
Radio & X-Ray Sources
EMISSION
FREQUENCY DEPENDENCE
HEATING
N56300* --Physics (Astrophysics & Cosmology)--Quasi-stellar
Radio & X-Ray Sources
SYNCHROTRON RADIATION