B-type emission-line stars with warm circumstellar dust

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 )
Web Site: http://library.uncg.edu/

Abstract: We selected a group of 11 B-type emission-line stars with large IR excesses, which show a steep flux decrease towards longer wave-lengths. Analysis of their observational characteristics has been carried out on the basis of the data collected from literature, results of our recent photometric and high-resolution spectroscopic observations. Possible nature and evolutionary state of the group objects are discussed.

Additional Information

Sheikina, T.A. Miroschnichenko, A.S. Corporon P. 2000. ASP Conference Series, 214, 303-308. B-type emission-line stars with warm circumstellar dust
Language: English
Date: 2000
B-type stars, Emission lines, Stars with warm dust, Stellar evolution

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