The Luminous B [e] Binary AS 381

UNCG Author/Contributor (non-UNCG co-authors, if there are any, appear on document)
Anatoly S. Miroshnichenko, Professor (Creator)
The University of North Carolina at Greensboro (UNCG )
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Abstract: We present the results of optical and near-IR spectroscopic and broadband multicolour photometric observations of the emission-line star AS 381. Its properties were found to be similar to those of Be stars with warm dust, a group of galactic objects recently defined by Sheikina et al. (2000). The spectrum of AS 381 indicates the presence of both a hot (early B-type) and a cool (K-type) star in the system.

Additional Information

Astronomy and Astrophysics 383, 171-181
Language: English
Date: 2002
stars: emission-line, Be, stars: individual: AS 381, techniques: spectroscopic, techniques: photometric

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