The transient X-ray source A0620-00 - Intensity variations and evidence for an 8 day periodicity

Details The transient X-ray source A0620-00 - Intensity variations and evidence for an 8 day periodicity The transient X-ray source A0620-00 - Intensity variations and evidence for an 8 day periodicity

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...210l.127m&link_type=abstract

Astrophysical Journal, vol. 210, Dec. 15, 1976, pt. 2, p. L127-L131.

Astronomy and Astrophysics

Astronomy

44

Binary Stars, Radiant Flux Density, Stellar Radiation, Variable Stars, X Ray Sources, Black Holes (Astronomy), Neutron Stars, Stellar Luminosity, Stellar Spectra, White Dwarf Stars, X Ray Stars

Scientific paper

The X-ray intensity of the transient source A0620-00 has been measured frequently with the SAS-3 X-ray Observatory from August 8, 1975 to February 13, 1976. This brightest of all known X-ray transients shows intensity variations on a time scale of days superposed on a general decline. Intensity data for the period from January 7 to February 13, 1976, show evidence of an approximate 7.8-day periodicity that may be the result of binary motion.

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