Optical identification of the transient X-ray source A1524-61

Details Optical identification of the transient X-ray source A1524-61 Optical identification of the transient X-ray source A1524-61

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mnras.178p..27m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 178, Feb. 1977, p. 27P-32P.

Astronomy and Astrophysics

Astronomy

14

Light Curve, Novae, X Ray Astronomy, X Ray Sources, Ariel 5 Satellite, Crab Nebula, Decay Rates, Identifying, Luminous Intensity, Optical Measurement, Radiant Flux Density, Star Distribution, Telescopes

Scientific paper

The identification of the transient X-ray source A1524-61 with a faint
optical nova is proposed. From consideration of the optical and X-ray
light curves, as well as the optical-to-X-ray luminosity ratio, this
object appears strikingly similar to the outstandingly bright X-ray nova
A0620-00 (=1975 Nova Mon = V616Mon).

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