Testing the forward modeling approach in asteroseismology: I. Seismic solutions for the hot B subdwarf Balloon 090100001 with and without a priori mode identification

Astronomy and Astrophysics

Volumn 488, Issue 2, 2008, Pages 685-696

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

^a UNIVERSITÉ DE TOULOUSE   (France)

^b UNIVERSITÉ DE MONTRÉAL   (Canada)

^c UNIVERSITY OF ARIZONA   (United States)

^d STScI   (United States)

^e EUROPEAN SOUTHERN OBSERVATORY   (Germany)

Author keywords

Stars: individual: Balloon 090100001; Stars: interiors; Stars: oscillations; Stars: subdwarfs

Indexed keywords

BALLOONS; PHOTOGRAPHY; SEISMOLOGY; SOLUTIONS; SPACECRAFT OBSERVATORIES; STARS;

MODE IDENTIFICATION; STARS: INDIVIDUAL: BALLOON 090100001; STARS: INTERIORS; STARS: OSCILLATIONS; STARS: SUBDWARFS;

IDENTIFICATION (CONTROL SYSTEMS);

EID: 50549087084     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809867     Document Type: Article

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