THE BM Ori system.: IV.: A new component of the system

被引：7
|
作者：
Vitrichenko, ÉA
Klochkova, VG
Tsymbal, VV
机构：
[1] Russian Acad Sci, Space Res Inst, Moscow 117901, Russia
[2] Russian Acad Sci, Special Astrophys Observ, Moscow 117901, Russia
[3] Taurian Natl Univ, Crimea, Ukraine
来源：
ASTROPHYSICS | 2006年 / 49卷 / 01期
关键词：
stars : eclipsing binary : Orion Trapezium;
D O I：
10.1007/s10511-006-0011-5
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Cross correlations between observed and synthetic spectra are used to discover yet another satellite of BM Ori with the following characteristics: effective temperature T-eff = 4000 K, radius R = 16R(circle dot), mass M = 1.8M(circle dot), spectral type K7 III, absolute bolometric stellar magnitude M-b = + 4(m).0, axial rotation velocity V sini = 85 km/s, and relative luminosity 0.005 near the V band.
引用
收藏
页码：96 / 104
页数：9
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