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
收藏
页码:205 / 225
页数:21
相关论文
共 29 条
[1]  
[Anonymous], 1985, GEN CATALOGUE VARIAB
[2]   SOUTHERN HEMISPHERE PHOTOMETRY .4. THE GALACTIC CLUSTER NGC 4755 [J].
ARP, HC ;
VANSANT, CT .
ASTRONOMICAL JOURNAL, 1958, 63 (08) :341-346
[3]  
ASLANOV AA, 1989, KATALOG TESNYKH DVOI
[4]  
BIBO EA, 1992, ASTRON ASTROPHYS, V260, P293
[5]   PHOTOELECTRIC PHOTOMETRY OF THE ASSOCIATION-III CEPHEI [J].
BLAAUW, A ;
HILTNER, WA .
ASTROPHYSICAL JOURNAL, 1959, 130 (01) :69-&
[6]   A SCANNED CCD SEARCH FOR CEPHEIDS AND OTHER VARIABLES IN CRUX AND CENTAURUS [J].
CALDWELL, JAR ;
KEANE, MJ ;
SCHECHTER, PL .
ASTRONOMICAL JOURNAL, 1991, 101 (05) :1763-1787
[7]  
CARBALLO R, 1992, ASTRON ASTROPHYS, V262, P106
[8]  
Dong Yisun, 1991, Acta Astrophysica Sinica, V11, P172
[9]   THE GALACTIC CLUSTER NGC 4755 (K-CRUCIS) [J].
FEAST, MW .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1963, 126 (01) :11-28
[10]  
FRIEDEMANN C, 1990, IAU INFORM B VAR STA, V3516