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Properties and nature of Be stars 30. Reliable physical properties of a semi-detached B9.5e+G8III binary BR CMi = HD 61273 compared to those of other well studied semi-detached emission-line binaries
- 1.0444996 - ASÚ 2016 RIV FR eng J - Journal Article
Harmanec, P. - Koubský, Pavel - Nemravová, J. - Royer, F. - Briot, D. - North, P. - Lampens, P. - Frémat, Y. - Yang, S. - Božić, H. - Kotková, Lenka - Škoda, Petr - Šlechta, Miroslav - Korčáková, D. - Wolf, M. - Zasche, P.
Properties and nature of Be stars 30. Reliable physical properties of a semi-detached B9.5e+G8III binary BR CMi = HD 61273 compared to those of other well studied semi-detached emission-line binaries.
Astronomy & Astrophysics. Roč. 573, January (2015), A107/1-A107/17. ISSN 0004-6361. E-ISSN 1432-0746
R&D Projects: GA ČR GD205/08/H005
Grant - others:GA ČR(CZ) GA205/06/0304; GA ČR(CZ) GAP209/10/0715
Institutional support: RVO:67985815
Keywords : close binaries * spectroscopic * emission-line
OECD category: Astronomy (including astrophysics,space science)
Impact factor: 5.185, year: 2015
we report the first detailed study of a new representative of this class of binaries, BR CMi, based on the analysis of radial velocities and multichannel photometry from several observatories, and compare its physical properties with those for other well-studied systems.
Permanent Link: http://hdl.handle.net/11104/0247434
Number of the records: 1