Eclipsing binaries as IRAS sources

被引:19
作者
Friedemann, C [1 ]
Gurtler, J [1 ]
Lowe, M [1 ]
机构
[1] MAX PLANCK GESELL,ARBEITSGRP STAUB STERNENTSTEHUNGSGEBIETEN,D-07745 JENA,GERMANY
来源
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1996年 / 117卷 / 02期
关键词
binaries; eclipsing; circumstellar matter; stars; carbon; infrared;
D O I
10.1051/aas:1996152
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In a systematic search we looked for coincidences in the positions of eclipsing binaries and IRAS point sources as evidence of a physical association. In a detailed discussion of the available optical and infrared data combined with model calculations, we show that 50-75% of the coincidences between eclipsing binaries and IRAS sources are real. We discuss a subsample of 44 stars in some detail and surveyed the vicinity of them on POSS and SRC/ESO atlases for possible optical counterparts and present identification maps. In the cases of BS Sco and V 718 Sco the infrared radiation may come from an accretion disk.
引用
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页码:205 / 225
页数:21
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