GJ 1230: A nearby triple system

被引：21

作者：

Gizis, JE

Reid, IN

机构：

[1] Palomar Observatory, 105-24, California Institute of Technology, Pasadena

来源：

ASTRONOMICAL JOURNAL | 1996年 / 111卷 / 01期

关键词：

D O I：

10.1086/117789

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present Keck HIRES and Palomar spectra of the nearby system GJ 1230. Henry ct al. [AJ, 108, 1437 (1994)] classified both the A and B components as M4.5 V and noted that the B component is apparently underluminous. High resolution spectra reveal that the A component is a short-period, near equal-mass binary. This fact, together with a slightly later classification for B and the kink in the HR diagram at M4.0-4.5 V, largely resolves the mystery of the luminosity discrepancy. (C) 1996 American Astronomical Society.

引用

页码：365 / 369

页数：5

共 16 条

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[2]

HAWLEY SL, 1905, UNPUB

[3]

Henry T. J., 1991, THESIS

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