The variable light curve of the X-ray transient EXO 0748 - 676

Details The variable light curve of the X-ray transient EXO 0748 - 676 The variable light curve of the X-ray transient EXO 0748 - 676

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987aj.....93..374s&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 93, Feb. 1987, p. 374-378. NSF-supported research.

Astronomy and Astrophysics

Astronomy

18

Light Curve, Variable Stars, Visible Spectrum, X Ray Stars, Stellar Color, Stellar Luminosity, Stellar Orbits, Stellar Spectrophotometry, Transient Response

Scientific paper

An optical light curve of the 3.8 hr eclipsing X-ray transient EXO 0748 - 676 was obtained in November 1985. The curve differs in shape from one observed in February 1985, although the overall brightness of the nova has not changed noticeably. No (B - V) color variation is found in the orbital cycle. Evidence is presented that one optical burst was observed. Possible interpretations of the variable light curve are discussed.

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