Astreroseismological results for the star V351 Ori

Details Astreroseismological results for the star V351 Ori Astreroseismological results for the star V351 Ori

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..895..224s&link_type=abstract

FIFTY YEARS OF ROMANIAN ASTROPHYSICS. AIP Conference Proceedings, Volume 895, pp. 224-227 (2007).

Astronomy and Astrophysics

Astrophysics

1

Pulsations, Oscillations, And Stellar Seismology, Pre-Main Sequence Objects, Young Stellar Objects And Protostars

Scientific paper

In this paper we present the results obtained for the star V351 Ori using CESAM evolutive model combined with the ROMOSC inversion method. The inversion method is based on a (O - C)2 minimum search for the observed modes combined with the nonadiabatic stability condition of the mode and assuming the range for Te given by observations.
The HR position obtained for the star is in the vicinity of the pms/postms common point, which lies far from the main sequence. A discussion about the evolutive status of the star (pms/postms) is also made.

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