1999A&AS..134..327D

Query : 1999A&AS..134..327D

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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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024 		#notes
1 V* V382 Cyg SB* 20 18 47.2202814912 +36 20 26.085111756 9.35 9.19 8.65     O6IVn+O5Vn 191 0
2 HD 193443 SB* 20 18 51.7093796362 +38 16 46.504188062 7.11 7.59 7.26     O8.5III:((f))+O9.2:IV: 142 0
3 HD 195407 Be* 20 29 47.7636491928 +36 58 49.368844488 7.47 8.13 7.80     B1Ve_shell 70 0

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