UBVRI Photometric Analysis of the Solar-Type Eclipsing Binary TYC 3034-299-1
Joint Authors
White, Jesse
Faulkner, Danny R.
Samec, Ronald G.
Jaso, Adam
Blum, Nicholas
Hamme, Walter Van
Source
ISRN Astronomy and Astrophysics
Issue
Vol. 2012, Issue 2012 (31 Dec. 2012), pp.1-11, 11 p.
Publisher
Hindawi Publishing Corporation
Publication Date
2012-03-11
Country of Publication
Egypt
No. of Pages
11
Main Subjects
Abstract EN
TYC 3034-0299-1 (CVn) is a magnetically active, contact binary, ROTSE variable.
UBVRcIc light curves are presented along with a period study and a simultaneous UBVRI light curve solution.
Our light curves show eclipse amplitudes of 0.72 and 0.62 mags (V) in the primary and secondary eclipses.
Modeled results include a dark spot region, found at longitude 51°, a 24% Roche lobe fill-out, and a mass ratio of 0.48.
A total eclipse is found to occur in the secondary eclipse making TYC 3034-0299-1 a W-type (less massive star is hotter) W UMa variable.
American Psychological Association (APA)
Samec, Ronald G.& Jaso, Adam& White, Jesse& Faulkner, Danny R.& Blum, Nicholas& Hamme, Walter Van. 2012. UBVRI Photometric Analysis of the Solar-Type Eclipsing Binary TYC 3034-299-1. ISRN Astronomy and Astrophysics،Vol. 2012, no. 2012, pp.1-11.
https://search.emarefa.net/detail/BIM-512566
Modern Language Association (MLA)
Samec, Ronald G.…[et al.]. UBVRI Photometric Analysis of the Solar-Type Eclipsing Binary TYC 3034-299-1. ISRN Astronomy and Astrophysics No. 2012 (2012), pp.1-11.
https://search.emarefa.net/detail/BIM-512566
American Medical Association (AMA)
Samec, Ronald G.& Jaso, Adam& White, Jesse& Faulkner, Danny R.& Blum, Nicholas& Hamme, Walter Van. UBVRI Photometric Analysis of the Solar-Type Eclipsing Binary TYC 3034-299-1. ISRN Astronomy and Astrophysics. 2012. Vol. 2012, no. 2012, pp.1-11.
https://search.emarefa.net/detail/BIM-512566
Data Type
Journal Articles
Language
English
Notes
Includes bibliographical references
Record ID
BIM-512566
