Bibcode
Casares, J.; Charles, P. A.
Bibliographical reference
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 255, March 1, 1992, p. 7-18.
Advertised on:
3
1992
Citations
24
Refereed citations
20
Description
Results of high-resolution optical spectroscopy of V404 Cyg (the optical
counterpart of the X-ray transient GS2023 + 338), conducted 13 months
after the May 1989 outburst are presented. The double-peaked H-alpha
line exhibits a strong S-wave modulation from which a periodicity of 5.7
hr is deduced. The level of the continuum is also modulated on the same
time-scale. This behavior is identified with the orbital period of the
system. There are also changes in the FWHM and peak separation, which
evolves from widening to subsequent shrinking. Such variations suggest a
very complex line profile consisting perphaps of several different
components.