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Improved basic physical properties of the Oe-star binary V1007 Sco
- 1.0124855 - ASU-R 20010108 RIV NL eng C - Conference Paper (international conference)
Mayer, P. - Harmanec, Petr - Lorenz, R. - Drechsel, H. - Eenens, P. - Corral, L. J. - Morrell, N.
Improved basic physical properties of the Oe-star binary V1007 Sco.
The influence of binaries on stellar population studies. Dordrecht: Kluwer, 2001 - (Vanbeveren, D.), s. 567-569. Astrophysics and space science library., 264.
[Influence of binaries on stellar population studies. Brusel (BE), 21.08.2000-25.08.2000]
R&D Projects: GA MŠMT ME 402
Institutional research plan: CEZ:AV0Z1003909
Keywords : hot stars * masses and radii * apsidal motion
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
The discovery of apsidal motion in the O star binary V1007 Sco with a period of 132 years is reported. New, more accurate orbital elements and light-curve solutions were also derived.
Permanent Link: http://hdl.handle.net/11104/0023114
Number of the records: 1