[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, S.K.
Fontaine, G.
Brassard, Pierre
Silvotti, R.
Van Grootel, Valérie ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie
Charpinet, Stéphane
Dhillon, V.S.
Marsh, T.R.
Language :
English
Title :
Pulsational Mode Identification Based on Chromatic Amplitude Behaviour: Recent Results for Rapidly Oscillating Subdwarf B Stars
Publication date :
October 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
