Photometric and spectroscopic observations of an optical candidate for the X-ray source H 0544 - 665

Details Photometric and spectroscopic observations of an optical candidate for the X-ray source H 0544 - 665 Photometric and spectroscopic observations of an optical candidate for the X-ray source H 0544 - 665

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.203..279v&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 203, Apr. 1983, p. 279-284. Research supported by the Nederlandse Organ

Astronomy and Astrophysics

Astronomy

7

B Stars, Magellanic Clouds, Stellar Spectra, Ubv Spectra, Variable Stars, X Ray Sources, Balmer Series, Electrophotometry, Stellar Color, Stellar Magnitude

Scientific paper

We present the results of spectroscopic and UBV observations of the brightest star in the error box of the X-ray source H 0544-665. This object is a B0-1 V star and a member of the LMC. It shows correlated variations in brightness and colour indices. We suggest that it is a Be-type star observed during a stage of low emission strength. Although a relation between this star and the X-ray source has still to be proven the present data add considerable support to the proposed identification.

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