VBLUW photometry of the high-latitude, eclipsing system V 748 CEN /= CEN X-4, tentatively/

Details VBLUW photometry of the high-latitude, eclipsing system V 748 CEN /= CEN X-4, tentatively/ VBLUW photometry of the high-latitude, eclipsing system V 748 CEN /= CEN X-4, tentatively/

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....73..183v&link_type=abstract

Astronomy and Astrophysics, vol. 73, no. 1-2, Mar. 1979, p. 183-189.

Astronomy and Astrophysics

Astrophysics

4

Eclipsing Binary Stars, Light Curve, Stellar Spectrophotometry, Ubv Spectra, X Ray Sources, Gas Streams, Giant Stars, Hot Stars, Infrared Spectrophotometers, Interstellar Extinction, M Stars, Stellar Envelopes

Scientific paper

VBLUW photometry of the high-latitude eclipsing binary V748 Cen, which has been tentatively identified with the transient X-ray source Cen X-4, is reported. It is found that the light curve is apparently not symmetric about the eclipse and that an extended system consisting of a shell and gas streams has an important effect on the binary's photometric properties. The nature of the binary and its two components is considered.

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