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- W1518263693 abstract "Very low-mass stars and brown dwarfs can undergo pulsational instability excited by central deuterium burning during the initial phases of their evolution. We present the results of evolutionary and nonadiabatic linear stability models that show the presence of unstable fundamental modes. The pulsation periods vary bewteen ~5 hr for a 0.1 Msun star and ~1 hr for a 0.02 M$_odot$ brown dwarf. The results are rather insensitive to variations in the input physics of the models. We show the location of the instability strip in the HR and c-m diagrams and discuss the observational searches for young pulsators in nearby star forming regions." @default.
- W1518263693 created "2016-06-24" @default.
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- W1518263693 date "2005-02-09" @default.
- W1518263693 modified "2023-09-27" @default.
- W1518263693 title "Pulsations induced by deuterium-burning in young brown dwarfs" @default.
- W1518263693 hasPublicationYear "2005" @default.
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