The secondaries of solar-type primaries. I. The radial velocities

被引：40

作者：

Abt, HA ^{[1
]}

Willmarth, D ^{[1
]}

机构：

[1] Kitt Peak Natl Observ, Tucson, AZ 85726 USA

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2006年 / 162卷 / 01期

关键词：

binaries : spectroscopic; binaries : visual; planetary systems; stars : statistics;

D O I：

10.1086/498095

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We studied for duplicity the 167 F7-G8 IV or V primaries within 25 pc of the Sun according to their Hipparcos parallaxes and between declinations of -30 degrees and +75 degrees. We obtained an average of 13 coude radial velocities with an accuracy of +/- 0.10 km s(-1). Combining these measures with published data, we obtained 39 single-lined and 12 double-lined binaries with orbital elements. This material will be combined in a later paper with the known visual binaries to derive the secondary mass frequencies.

引用

页码：207 / 226

页数：20