Improved basic physical properties of the Oe-star binary V1007 Sco
1.
SYSNO ASEP
0124855
Document Type
C - Proceedings Paper (int. conf.)
R&D Document Type
Conference Paper
Title
Improved basic physical properties of the Oe-star binary V1007 Sco
Author(s)
Mayer, P. (CZ) Harmanec, Petr (ASU-R) Lorenz, R. (DE) Drechsel, H. (DE) Eenens, P. (MX) Corral, L. J. (ES) Morrell, N. (AR)
Source Title
The influence of binaries on stellar population studies / Vanbeveren D.. - Dordrecht : Kluwer, 2001
Pages
s. 567-569
Number of pages
3 s.
Action
Influence of binaries on stellar population studies
Event date
21.08.2000-25.08.2000
VEvent location
Brusel
Country
BE - Belgium
Event type
WRD
Language
eng - English
Country
NL - Netherlands
Keywords
hot stars ; masses and radii ; apsidal motion
Subject RIV
BN - Astronomy, Celestial Mechanics, Astrophysics
R&D Projects
ME 402 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
CEZ
AV0Z1003909 - ASU-R
Annotation
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.
