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)
- Institution
- The University of North Carolina at Greensboro (UNCG )
- Web Site: http://library.uncg.edu/
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.
The Luminous B [e] Binary AS 381
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Created on 1/1/2002
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Additional Information
- Publication
- Astronomy and Astrophysics 383, 171-181
- Language: English
- Date: 2002
- Keywords
- stars: emission-line, Be, stars: individual: AS 381, techniques: spectroscopic, techniques: photometric