Binarity among objects with the Be and B[e] phenomena

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7358

Title:	Binarity among objects with the Be and B[e] phenomena
Authors:	Miroshnichenko, A. S Zharikov, S.V Korcakova, D Manset, N Mennickent, R Khokhlov, S. A Danford, S Raj, A Zakhozhay, O.V
Keywords:	Stars: emission-line Be B[e] Stars: binaries: spectroscopic
Issue Date:	Mar-2020
Publisher:	Astronomical Institute of the Slovak Academy of Sciences
Citation:	Contributions of the Astronomical Observatory Skalnaté Pleso, Vol. 50, No. 2, pp. 513-517.
Abstract:	Many B-type stars exhibit two phenomena that are symbolized Be and B[e]. The former refers to presence of a circumstellar gaseous disk without significant circumstellar dust, while the latter have dust. Although neither phenomenon is fully understood, growing evidence suggests that binarity plays an important role. Recent results on Be and B[e] binaries, along with methods of their discovery, are reviewed.
Description:	Open Access
URI:	http://prints.iiap.res.in/handle/2248/7358
ISSN:	1336-0337
Appears in Collections:	IIAP Publications

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