Nonradial Oscillations on a Pre-Main-Sequence Star

Details Nonradial Oscillations on a Pre-Main-Sequence Star Nonradial Oscillations on a Pre-Main-Sequence Star

Jan 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007apj...655..342z&link_type=abstract

The Astrophysical Journal, Volume 655, Issue 1, pp. 342-344.

Astronomy and Astrophysics

Astronomy

8

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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