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- W2891638877 abstract "The most violent strange mode pulsations (SMPs) are expected in classical WR stars, the bare, compact helium-burning cores of evolved massive stars, where SMPs are predicted to manifest themselves in cyclic photometric variability with periods ranging from minutes to hours and amplitudes in the several to tens of mmag range. Since WR,2 is one of the hottest WR stars known, it should make it an excellent candidate for SMPs. However, our high-precision near infrared photometric campaign shows no periodic variations with an amplitude higher than 2.5 mmag on a timescale of ~6 hours, which is more than an order of magnitude smaller than the theoretical predictions." @default.
- W2891638877 created "2018-09-27" @default.
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- W2891638877 date "2018-09-10" @default.
- W2891638877 modified "2023-10-18" @default.
- W2891638877 title "No detection of Strange Mode Pulsations in massive prime candidate" @default.
- W2891638877 hasPublicationYear "2018" @default.
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