Recurrent X-ray outbursts from Aquila X-1

Details Recurrent X-ray outbursts from Aquila X-1 Recurrent X-ray outbursts from Aquila X-1

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977natur.265..606k&link_type=abstract

Nature, vol. 265, Feb. 17, 1977, p. 606, 607. Research supported by the University of Maryland.

Astronomy and Astrophysics

Astronomy

25

Binary Stars, Dwarf Stars, Novae, X Ray Sources, Ariel Satellites, Spaceborne Astronomy, Variable Stars, X Ray Astronomy, X Ray Stars

Scientific paper

Ariel V All-Sky Monitor observations of Aql X-1 are reported and compared with previous observations that indicate the existence of 'low' and 'high' intensity states. All the data considered are shown to be consistent with flaring episodes having a mean flare interval of 435 days with an rms scatter of about 10%. It is suggested that the observations are most easily interpreted in terms of an 'X-ray dwarf nova' binary of the type proposed for the transient X-ray source A0620-00. Constraints on more detailed features of the source model are discussed.

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