Testing the forward modeling approach in asteroseismology II. Structure and internal dynamics of the hot B subdwarf component in the close eclipsing binary system PG 1336-018

Astronomy and Astrophysics

Volumn 489, Issue 1, 2008, Pages 377-394

  Charpinet, S ^a   Van Grootel, V ^a,b   Reese, D ^c   Fontaine, G ^b   Green, E M ^d   Brassard, P ^b   Chayer, P ^e  

^a UNIVERSITÉ DE TOULOUSE   (France)

^b UNIVERSITÉ DE MONTRÉAL   (Canada)

^c UNIVERSITY OF SHEFFIELD   (United Kingdom)

^d UNIVERSITY OF ARIZONA   (United States)

^e STScI   (United States)

Author keywords

Stars: binaries: close; Stars: individual: PG 1336 018; Stars: interiors; Stars: oscillations; Stars: rotation; Stars: subdwarfs

Indexed keywords

CURVE FITTING; OPERATIONS RESEARCH; ROTATION; SEISMOLOGY; SYSTEMS (METALLURGICAL);

ASTEROSEISMOLOGY; BINARY SYSTEMS; FORWARD MODELLING; INTERNAL DYNAMICS; INTERNAL ROTATION; LIGHT CURVES; OPTIMAL MODELING; OPTIMIZATION TECHNIQUES; PARAMETER SPACES; POSSIBLE SOLUTIONS; SEISMIC ANALYSIS; SEISMIC MODELING; STARS: BINARIES: CLOSE; STARS: INDIVIDUAL: PG 1336-018; STARS: INTERIORS; STARS: OSCILLATIONS; STARS: ROTATION; STARS: SUBDWARFS; STELLAR ROTATION; STRINGENT TEST;

DYNAMICS;

EID: 52649179913     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809907     Document Type: Article

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