Identification of the optical counterpart of the X-ray source V0332 + 53

Details Identification of the optical counterpart of the X-ray source V0332 + 53 Identification of the optical counterpart of the X-ray source V0332 + 53

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...132l...8b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 132, no. 2, March 1984, p. L8.

Astronomy and Astrophysics

Astrophysics

18

Stellar Spectra, Variable Stars, X Ray Sources, Astronomical Photometry, H Alpha Line, Position (Location)

Scientific paper

The optical counterpart of the X-ray transient V0332+53 is a star of
magnitudes V = 15.13 and B-V = 2.31. The line Hα has a P-Cygni
profile with the absorption component at -1400 km/s. The possibility of
a 2.198 s optical periodicity, at 3.4σ level, is investigated.

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