Spot activity of the new WUMa-type variable GSC3599-2569 View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2015-01

AUTHORS

S. Yu. Gorda, A. P. Lyaptsev, A. M. Sobolev

ABSTRACT

A new A-subtype W UMa eclipsing binary is found in the vicinity of the young bright massive variable V 645 Cyg. Over the four-year long observation interval (2009–2013), the star’s light curve shifted along the magnitude axis with an amplitude of 0ṃ08, and the depths of its minima varied by up to 0ṃ055. The parameters of the components of this new eclipsing system are estimated, and indications of long-term flux variation with a period of 940 days are found. It is suggested that such variations can be explained by the spot activity of the components. The parameters of the spot structure are determined for the case of maximum spot activity. More... »

PAGES

109-116

Journal

TITLE

Astrophysical Bulletin

ISSUE

1

VOLUME

70

Author Affiliations

Identifiers

URI

http://scigraph.springernature.com/pub.10.1134/s1990341315010125

DOI

http://dx.doi.org/10.1134/s1990341315010125

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1009581167


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