中大學術數位典藏-NCU Institutional Repository:Item 987654321/101875
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    题名: Variable stars in young open star cluster NGC 7380
    作者: 陳文屏;Lata, Sneh;Pandey, A. K.;Panwar, Neelam;Chen, W. P.;Samal, M. R.;Pandey, J. C.
    贡献者: 理學院天文研究所
    关键词: Astrophysics;B stars;Clusters;Color;Colour;Physics;Pulsars;Star & galaxy formation;Star clusters;Stars;Time series;Variable stars
    日期: 2016-03-01
    上传时间: 2026-04-21 14:49:07 (UTC+8)
    出版者: Oxford University Press;London: Oxford University Press
    摘要: 摘要: We present time series photometry of 57 variable stars in the cluster region NGC 7380. The association of these variable stars with the cluster NGC 7380 has been established on the basis of two colour diagrams and colour–magnitude diagrams. 17 stars are found to be main-sequence variables, which are mainly B-type stars and are classified as slowly pulsating B stars, β Cep or δ Scuti stars. Some of them may belong to new class variables as discussed by Mowlavi et al. and Lata et al. Present sample also contains 14 pre-main-sequence stars, whose ages and masses are found to be mostly ≲5 Myr and range 0.60 ≲ M/M⊙ ≲ 2.30 and hence should be T-Tauri stars. About half of the weak-line T-Tauri stars are found to be fast rotators with a period of ≲2 d as compared to the classical T-Tauri stars. Some of the variables belong to the field star population.
    出版者: London: Oxford University Press
    出版日期: 2016-03-01
    出處: Monthly notices of the Royal Astronomical Society, 2016-03, Vol.456 (3), p.2505-2517
    資源來源: Alma/SFX Local Collection
    版權: 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society 2015
    版權: Copyright Oxford University Press, UK Mar 1, 2016
    版權: licence_http://creativecommons.org/publicdomain/zero
    識別號: ISSN: 0035-8711
    識別號: ISSN: 1365-8711
    識別號: ISSN: 1365-2966
    識別號: EISSN: 1365-2966
    識別號: DOI: 10.1093/mnras/stv2800
    显示于类别:[天文研究所] 期刊論文

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