THEORETICAL p-MODE OSCILLATION FREQUENCIES FOR THE RAPIDLY ROTATING Delta d SCUTI STAR Delta a OPHIUCHI

A rotating, two-dimensional stellar model is evolved to match the approximate conditions of Delta *a Oph. Both axisymmetric and nonaxisymmetric oscillation frequencies are computed for two-dimensional rotating models which approximate the properties of Delta *a Oph. These computed frequencies are co...

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Veröffentlicht in:	The Astrophysical journal 2011-11 (1), p.jQuery1323901434395='48'-jQuery1323901434395='48'
1. Verfasser:	Deupree, Robert G
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext
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