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Study of classical Be stars in open clusters older than 100 Myr

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dc.contributor.author Jagadeesh, Madhu Kashyap
dc.contributor.author Blesson, Mathew
dc.contributor.author Paul, K. T
dc.contributor.author Banerjee, Gourav
dc.contributor.author Subramaniam, A
dc.contributor.author Arun, R
dc.date.accessioned 2022-01-20T06:47:58Z
dc.date.available 2022-01-20T06:47:58Z
dc.date.issued 2021-10
dc.identifier.citation Journal of Astrophysics and Astronomy, Vol. 42, No. 2, 109 en_US
dc.identifier.issn 0973-7758
dc.identifier.uri http://hdl.handle.net/2248/7909
dc.description Restricted access en_US
dc.description The original publication is available at springerlink.com
dc.description.abstract We 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.iso en en_US
dc.publisher Springer en_US
dc.relation.uri https://doi.org/10.1007/s12036-021-09780-w
dc.rights © Indian Academy of Sciences
dc.subject Classical Be stars en_US
dc.subject Slitless spectroscopy en_US
dc.subject Spectral type en_US
dc.subject Color en_US
dc.subject Color diagram en_US
dc.subject Open clusters en_US
dc.title Study of classical Be stars in open clusters older than 100 Myr en_US
dc.type Article en_US


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