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Oscillations in Young Stellar Objects
Published online by Cambridge University Press: 12 April 2016
Abstract
We report the discovery of periodicities in the light curve of the Herbig Ae star V346 Ori. We interpret these variations as the superposition of at least two signals with periods P1=42±6 min and P2=68±12 min resulting from stellar oscillations. The computation of linear non-adiabatic pulsation models for Pre-Main Sequence (PMS) stars reproduces these periods for a 1.5 M⊙ star with Teff= 7300 K and log L/L⊙= 0.74, pulsating in the fundamental and second overtones.
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- Part 2.4. Delta Scuti Stars
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- Copyright © Astronomical Society of the Pacific 2002