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