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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7358
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dc.contributor.authorMiroshnichenko, A. S-
dc.contributor.authorZharikov, S.V-
dc.contributor.authorKorcakova, D-
dc.contributor.authorManset, N-
dc.contributor.authorMennickent, R-
dc.contributor.authorKhokhlov, S. A-
dc.contributor.authorDanford, S-
dc.contributor.authorRaj, A-
dc.contributor.authorZakhozhay, O.V-
dc.date.accessioned2020-11-26T15:04:17Z-
dc.date.available2020-11-26T15:04:17Z-
dc.date.issued2020-03-
dc.identifier.citationContributions of the Astronomical Observatory Skalnaté Pleso, Vol. 50, No. 2, pp. 513-517.en_US
dc.identifier.issn1336-0337-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/7358-
dc.descriptionOpen Accessen_US
dc.description.abstractMany 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.isoenen_US
dc.publisherAstronomical Institute of the Slovak Academy of Sciencesen_US
dc.relation.urihttps://doi.org/10.31577/caosp.2020.50.2.513-
dc.rights© Astronomical Institute of the Slovak Academy of Sciences-
dc.subjectStars: emission-lineen_US
dc.subjectBeen_US
dc.subjectB[e]en_US
dc.subjectStars: binaries: spectroscopicen_US
dc.titleBinarity among objects with the Be and B[e] phenomenaen_US
dc.typeArticleen_US
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