Published May 2011 | Version v1
Journal article

PERIOD CHANGES AND FOUR-COLOR LIGHT CURVES OF ACTIVE CONTACT BINARY VW BOOTIS

  • 1. National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, P.O. Box 110, 650011 Kunming (China)

Description

The secured four-color light curves of VW Boo were analyzed with the 2003 version of the Wilson-Devinney code. It is confirmed that VW Boo is a shallow W-type contact binary system with a degree of contact factor f = 10.8%(± 0.5%). Two dark spots were found on the massive cool component this time. They cause an unequal depth of the two maxima. A period investigation based on all available visual, photographic, CCD, and photoelectric data shows that the period of the system includes a long-term decrease (dP/dt = -1.454 x 10-7 days yr-1) and an oscillation (A3 = 0.0059 days; T3 = 25.96 years). These may be caused by mass transfer, angular momentum loss, and cyclic magnetic activity.

Availability note (English)

Available from http://dx.doi.org/10.1088/0004-6256/141/5/147

Additional details

Identifiers

Publishing Information

Journal Title
Astronomical Journal (New York, N.Y. Online)
Journal Volume
141
Journal Issue
5
Journal Page Range
[14 p.]
ISSN
1538-3881

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
43060701
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ANGULAR MOMENTUM; CHARGE-COUPLED DEVICES; COLOR; MASS TRANSFER; PHOTOGRAPHY; STAR EVOLUTION; STARS
Descriptors DEC
EVOLUTION; OPTICAL PROPERTIES; ORGANOLEPTIC PROPERTIES; PHYSICAL PROPERTIES; SEMICONDUCTOR DEVICES