Stellar variability in open clusters: II. Discovery of a new period-luminosity relation in a class of fast-rotating pulsating stars in NGC 3766

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[1] Mowlavi, N.
[2] Saesen, S.
[3] Semaan, T.
[4] Eggenberger, P.
[5] Barblan, F.
[6] Eyer, L.
[7] Ekström, S.
[8] Georgy, C.
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| 1600年 / EDP Sciences卷 / 595期
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  • [1] Stellar variability in open clusters II. Discovery of a new period-luminosity relation in a class of fast-rotating pulsating stars in NGC 3766
    Mowlavi, N.
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    Semaan, T.
    Eggenberger, P.
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    Ekstrom, S.
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    ASTRONOMY & ASTROPHYSICS, 2016, 595
  • [2] Period-luminosity relations of fast-rotating B-type stars in the young open cluster NGC 3766
    Saio, H.
    Ekstrom, S.
    Mowlavi, N.
    Georgy, C.
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    Eggenberger, P.
    Semaan, T.
    Salmon, S. J. A. J.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2017, 467 (04) : 3864 - 3873
  • [3] Stellar variability in open clusters I. A new class of variable stars in NGC 3766
    Mowlavi, N.
    Barblan, F.
    Saesen, S.
    Eyer, L.
    ASTRONOMY & ASTROPHYSICS, 2013, 554
  • [4] Are the stars of a new class of variability detected in NGC 3766 fast rotating SPB stars?
    Salmon, S. J. A. J.
    Montalban, J.
    Reese, D. R.
    Dupret, M-A
    Eggenberger, P.
    NEW WINDOWS ON MASSIVE STARS: ASTEROSEISMOLOGY, INTERFEROMETRY AND SPECTROPOLARIMETRY, 2014, 307 : 188 - 193
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