Nonradial Oscillations on a Pre-Main-Sequence Star

Astronomy and Astrophysics – Astronomy

Scientific paper

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Stars: Evolution, Stars: Oscillations, Stars: Pre-Main-Sequence

Scientific paper

We show that the modes observed on the pulsating pre-main-sequence (PMS) star NGC 6383 170 can be interpreted as a combination of radial and nonradial p-modes. Using a dense grid of PMS models and oscillation spectra, we have identified models that match the observed oscillation spectrum within 1 σ of the frequency uncertainties and are consistent with the star's position in the H-R diagram.

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