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

Astronomy and Astrophysics

Volumn 506, Issue 1, 2009, Pages 189-201

  Reese, D R ^a   MacGregor, K B ^b   Jackson, S ^b   Skumanich, A ^b   Metcalfe, T S ^b  

^a UNIVERSITY OF SHEFFIELD   (United Kingdom)

^b NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

Author keywords

Stars: oscillations; Stars: rotation

Indexed keywords

OPTICAL RESONATORS; ROTATION; STARS;

ASYMPTOTIC PATTERNS; GROUND-BASED NETWORK; MODE IDENTIFICATION; SELF-CONSISTENT FIELD METHOD; SELF-CONSISTENT-FIELD METHODS; STARS: OSCILLATION; STARS: ROTATION; VARIATIONAL PRINCIPLES;

WHISPERING GALLERY MODES;

EID: 84977487999     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811510     Document Type: Article

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