Probing the driving region in hot subdwarf stars through nonadiabatic asteroseismology: The principle of the method

Astronomy and Astrophysics

Volumn 493, Issue 2, 2009, Pages 595-600

  Charpinet, S ^a   Fontaine, G ^b   Brassard, P ^b  

^a UNIVERSITÉ DE TOULOUSE   (France)

^b UNIVERSITÉ DE MONTRÉAL   (Canada)

Author keywords

Stars: oscillations; Stars: subdwarfs

Indexed keywords

CHEMICAL ELEMENTS; HEAVY METALS; MOTION ESTIMATION;

ASTEROSEISMOLOGY; CHEMICAL COMPOSITIONS; DIFFUSIVE PROCESS; DOMINANT CONTRIBUTIONS; HEAVY ELEMENTS; IRON ENRICHMENTS; MIXING PROCESS; MODEL EXPERIMENTS; NON-ADIABATIC; PHYSICAL PROCESS; STARS: OSCILLATIONS; STARS: SUBDWARFS; STELLAR ENVELOPES; SUBDWARF STARS; TEST CASE; UNSTABLE MODES;

STARS;

EID: 59049086324     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810305     Document Type: Article

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