A near-IR study of the X-ray transient V0332+53

Details A near-IR study of the X-ray transient V0332+53 A near-IR study of the X-ray transient V0332+53

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.226..455c&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 226, May 15, 1987, p. 455-460.

Astronomy and Astrophysics

Astronomy

13

B Stars, Infrared Astronomy, Neutron Stars, X Ray Binaries, Near Infrared Radiation, Stellar Envelopes, Stellar Oscillations, X Ray Sources

Scientific paper

Near-infrared (JHKL') observations have been obtained of the binary system V0332+53. This is an X-ray transient consisting of a Be star in partnership with a neutron star. The IR data reveal a spectral component, separate from the optical emission, which undergoes changes on a time-scale of years. The possible origin of this IR component is discussed and it is suggested that the most likely interpretation is emission from a circumstellar gas cloud.

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