MX 1313+29 - A compact source of very low energy X-rays in Coma Berenices

Details MX 1313+29 - A compact source of very low energy X-rays in Coma Berenices MX 1313+29 - A compact source of very low energy X-rays in Coma Berenices

Jan 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...203l..21h&link_type=abstract

Astrophysical Journal, vol. 203, Jan. 1, 1976, pt. 2, p. L21-L24.

Astronomy and Astrophysics

Astrophysics

54

Brightness Temperature, Hot Stars, White Dwarf Stars, X Ray Sources, Satellite-Borne Instruments, Spaceborne Telescopes, Spectrum Analysis, X Ray Telescopes

Scientific paper

A compact X-ray source near the North Galactic Pole has been detected with the low-energy X-ray telescope aboard the SAS-3 satellite. The spectral temperature of the source is less than 1 million K, and the energy flux at the earth is 3 by 10 to the -10th power erg/sq cm/sec above 0.1 keV. The flux appeared to be constant both on short time scales (10-1000 s), and over the interval from the first SAS-3 observation (June 12, 1975) to the latest (July 15, 1975). The possible identification of this source with the hot white dwarf HZ 43 is discussed.

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