Near-IR photometry of southern X-ray binary systems

被引：9

作者：

Coe, MJ

Buckley, DAH

Fabregat, J

Steele, LA

Still, MD

Torrejon, JM

机构：

[1] SAAO,ZA-7935 OBSERVATORY,SOUTH AFRICA

[2] UNIV VALENCIA,DEPT ASTRON,E-46100 BURJASSOT,SPAIN

[3] LIVERPOOL JOHN MOORES UNIV,ASTROPHYS GRP,LIVERPOOL L3 3AF,MERSEYSIDE,ENGLAND

[4] UNIV ST ANDREWS,ST ANDREWS KY16 9SS,FIFE,SCOTLAND

来源：

ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1997年 / 126卷 / 02期

关键词：

stars; binaries; X-rays;

D O I：

10.1051/aas:1997260

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We report LR measurements of 30 optical counterparts to a group of possible and probable High Mass X-ray Binaries (HMXRBs). In the majority of the systems these measurements represent the first reported LR flux values. In common with many other similar systems, the results show the presence of a strong, frequently variable IR signal. The implications of some of the results are discussed.

引用

页码：237 / 240

页数：4

共 30 条

[1] DEEP EINSTEIN X-RAY IMAGERY OF THE SMALL MAGELLANIC CLOUD [J].