Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7909
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dc.contributor.authorJagadeesh, Madhu Kashyap-
dc.contributor.authorBlesson, Mathew-
dc.contributor.authorPaul, K. T-
dc.contributor.authorBanerjee, Gourav-
dc.contributor.authorSubramaniam, A-
dc.contributor.authorArun, R-
dc.date.accessioned2022-01-20T06:47:58Z-
dc.date.available2022-01-20T06:47:58Z-
dc.date.issued2021-10-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 42, No. 2, 109en_US
dc.identifier.issn0973-7758-
dc.identifier.urihttp://hdl.handle.net/2248/7909-
dc.descriptionRestricted accessen_US
dc.descriptionThe original publication is available at springerlink.com-
dc.description.abstractWe performed the slitless spectroscopic survey to identify classical Be (CBe) stars in open clusters older than 100 Myr. Observing a sample of 71 open clusters, we identified 13 CBe stars in 11 open clusters, one of, which (TYC 2679-432-1) is a new detection. The 13 CBe stars show both Ha in emission and IR excess, which confirm that they possess gaseous circumstellar discs. Two more CBe stars are found to exhibit Ha in absorption for the first time, indicating that might be passing through disc-less episode presently. The spectral-type estimation is done for all these 15 stars and it is noticed that they belong to B0.5–B8 type. Moreover, we found that the distribution of our sample is peaking near late B-types as expected.en_US
dc.language.isoenen_US
dc.publisherSpringeren_US
dc.relation.urihttps://doi.org/10.1007/s12036-021-09780-w-
dc.rights© Indian Academy of Sciences-
dc.subjectClassical Be starsen_US
dc.subjectSlitless spectroscopyen_US
dc.subjectSpectral typeen_US
dc.subjectColoren_US
dc.subjectColor diagramen_US
dc.subjectOpen clustersen_US
dc.titleStudy of classical Be stars in open clusters older than 100 Myren_US
dc.typeArticleen_US
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