Astron. Astrophys. Suppl. Ser.
Volume 117, Number 2, June I 1996
|Page(s)||205 - 225|
|Published online||15 June 1996|
Eclipsing binaries as IRAS sources
Universitäts–Sternwarte, Schillergäßchen 2, D-07745 Jena, Germany
2 Max-Planck-Gesellschaft, Arbeitsgruppe “Staub in Sternentstehungsgebieten", Schillergäßchen 2-3, D-07745 Jena, Germany
Send offprint request to: C. Friedemann
Accepted: 11 November 1995
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.
Key words: binaries: eclipsing / circumstellar matter / stars: carbon / infrared: stars
© European Southern Observatory (ESO), 1996