Abstract
The first complete CCD BVRI-filter light curves of the eclipsing near-contact binary V387 Cyg were obtained during 5 nights in 2004 at Kryoneri Observatory, Greece. Their analysis with the W-D program indicates a semidetached configuration with possible cool spots, although no O’ Connell effect is present and a strong asymmetry after Min II can be explained assuming either a strong flare or circumstellar matter.
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
References
Baldinelli, L., Maitan, A.: IBVS No. 5220 (2002)
Berthold, T.: IBVS No. 1203 (1976)
Brancewicz, H. K., Dworak, T. Z.: AcA 30, 501 (1980)
Manimanis, V.N., Niarchos, P.G.: IBVS No. 5624 (2005)
Morgenroth, V.O.: AN 255, 425 (1935)
Nelson, R.H.: IBVS No. 5040 (2001)
Nelson, R.H.: IBVS No. 5371 (2001)
Prša, A., Zwitter, T.: ApJ 628, 426 (2005)
Shaw, J.S.: Mem. S.A. Ital. 65, 95 (1994)
Author information
Authors and Affiliations
Corresponding author
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2006 Springer Science+Business Media B.V.
About this chapter
Cite this chapter
Manimanis, V.N., Niarchos, P.G. (2006). The Near-Contact System V387 Cygni: BVRI Photometry and Modelling. In: Giménez, À., Guinan, E., Niarchos, P., Rucinski, S. (eds) Close Binaries in the 21st Century: New Opportunities and Challenges. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-5027-5_15
Download citation
DOI: https://doi.org/10.1007/978-1-4020-5027-5_15
Received:
Accepted:
Publisher Name: Springer, Dordrecht
Print ISBN: 978-1-4020-5026-8
Online ISBN: 978-1-4020-5027-5
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)