Pulsation modes in rapidly rotating stellar models based on the self-consistent field method (2009)

First Author: Reese D
Attributed to:  Structure and dynamics of solar interior and other stars funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/200811510

Publication URI: http://dx.doi.org/10.1051/0004-6361/200811510

Type: Journal Article/Review

Parent Publication: Astronomy & Astrophysics

Issue: 1