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

dc.contributor.author	Miroshnichenko, A. S
dc.contributor.author	Zharikov, S.V
dc.contributor.author	Korcakova, D
dc.contributor.author	Manset, N
dc.contributor.author	Mennickent, R
dc.contributor.author	Khokhlov, S. A
dc.contributor.author	Danford, S
dc.contributor.author	Raj, A
dc.contributor.author	Zakhozhay, O.V
dc.date.accessioned	2020-11-26T15:04:17Z
dc.date.available	2020-11-26T15:04:17Z
dc.date.issued	2020-03
dc.identifier.citation	Contributions of the Astronomical Observatory Skalnaté Pleso, Vol. 50, No. 2, pp. 513-517.	en_US
dc.identifier.issn	1336-0337
dc.identifier.uri	http://prints.iiap.res.in/handle/2248/7358
dc.description	Open Access	en_US
dc.description.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.	en_US
dc.language.iso	en	en_US
dc.publisher	Astronomical Institute of the Slovak Academy of Sciences	en_US
dc.relation.uri	https://doi.org/10.31577/caosp.2020.50.2.513
dc.rights	© Astronomical Institute of the Slovak Academy of Sciences
dc.subject	Stars: emission-line	en_US
dc.subject	Be	en_US
dc.subject	B[e]	en_US
dc.subject	Stars: binaries: spectroscopic	en_US
dc.title	Binarity among objects with the Be and B[e] phenomena	en_US
dc.type	Article	en_US