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

页码：96 / 104

页数：9

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