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/10.48550/arxiv.0903.4854
Publication URI: https://arxiv.org/abs/0903.4854
Type: Other