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Pulsational Mode Identification Based on Chromatic Amplitude Behaviour: Recent Results for Rapidly Oscillating Subdwarf B Stars
Randall, Suzanna K; Fontaine, Gilles; Brassard, Pierre et al.
2012In Astronomical Society of the Pacific Conference Series, 462 (232)
 

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Abstract :
[en] We present recent results from mode identification based on the amplitude-wavelength behaviour for three rapidly pulsating subdwarf B stars: HS 2201+2610, EC 11583-2708 and EC 20338-1925.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Randall, Suzanna K
Fontaine, Gilles
Brassard, Pierre
Silvotti, Roberto
Van Grootel, Valérie  ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie
Charpinet, Stéphane
Dhillon, Vik S
Marsh, Tom R.
Language :
English
Title :
Pulsational Mode Identification Based on Chromatic Amplitude Behaviour: Recent Results for Rapidly Oscillating Subdwarf B Stars
Publication date :
September 2012
Event name :
Progress in Solar/Stellar Physics with Helio- and Asteroseismology
Event organizer :
H. Shibahashi
Event place :
Hakone, Japan
Event date :
13-17 Mars 2011
Audience :
International
Journal title :
Astronomical Society of the Pacific Conference Series
ISSN :
1050-3390
Publisher :
Astronomical Society of the Pacific, San Francisco, United States - California
Volume :
462
Issue :
232
Available on ORBi :
since 18 March 2014

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