Revised Photometric Elements of Qy-Aquilae V388-CYGNI and Hs-Herculis

Details Revised Photometric Elements of Qy-Aquilae V388-CYGNI and Hs-Herculis Revised Photometric Elements of Qy-Aquilae V388-CYGNI and Hs-Herculis

May 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ap%26ss..76..111g&link_type=abstract

Astrophysics and Space Science, Volume 76, Issue 1, pp.111-118

Astronomy and Astrophysics

Astrophysics

9

Scientific paper

Using Wood's model we have reanalyzed the light curves of the eclipsing binaries QY Aql, V388 Cyg, and HS Her. For QY Aql and HS Her our photometric solutions substantially confirm previous results, thus respectively supporting ansd-d classification and a main sequence detached view. On the other hand, significantly different photometric elements have been derived for V388 Cyg, which is likely to be an evolved contact binary.

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