SIMBAD references

1999A&AS..134..327D - Astron. Astrophys., Suppl. Ser., 134, 327-331 (1999/January-2)

The early type contact binary system V382 Cygni.

DEGIRMENCI O.L., SEZER C., DEMIRCAN O., ERDEM A., OZDEMIR S., AK H. and ALBAYRAK B.

Abstract (from CDS):

New photometric data set of the early type contact binary V382 Cyg have been analyzed with emphasis on determining the photometric mass ratio of the system. The result (q=0.68) supports the value given by Popper & Hill (1991AJ....101..600P). A study of the system using new data shows a period increase of about 3.28s per century, which corresponds to a very large rate ∼5.0x10–6M☉/yr of mass transfer from the less massive to the more massive component under the conservative mass transfer hypothesis.

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Journal keyword(s): stars: binaries: eclipsing - stars: individual: V382 Cyg

Simbad objects: 3

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