Observations of a transient X-ray source with a period of 104 S

Details Observations of a transient X-ray source with a period of 104 S Observations of a transient X-ray source with a period of 104 S

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975natur.256..628r&link_type=abstract

Nature, vol. 256, Aug. 21, 1975, p. 628-630.

Astronomy and Astrophysics

Astronomy

125

Crab Nebula, Light Curve, Spaceborne Astronomy, Variable Stars, X Ray Sources, Dwarf Stars, Radiant Flux Density, Stellar Radiation, X Ray Stars

Scientific paper

Observational data obtained by Ariel V are analyzed for the X-ray source A 0535 + 26, which varies with a period of 104 sec and has a very flat spectrum in the range from 3 to 7 keV. The observed count rate of this source is given together with its position (90% confidence), and periodic features at different frequencies are discussed. The light curve is shown to exhibit no signs of eclipses, and indications are found for increased absorption during the growth phase of the X-ray intensity.

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