Reference : Pulsational Mode Identification Based on Chromatic Amplitude Behaviour: Recent Result...
Scientific congresses and symposiums : Paper published in a journal
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/164375
Pulsational Mode Identification Based on Chromatic Amplitude Behaviour: Recent Results for Rapidly Oscillating Subdwarf B Stars
English
Randall, Suzanna K []
Fontaine, Gilles []
Brassard, Pierre []
Silvotti, Roberto []
Van Grootel, Valérie mailto [Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie >]
Charpinet, Stéphane []
Dhillon, Vik S []
Marsh, Tom R. []
Sep-2012
Astronomical Society of the Pacific Conference Series
Astronomical Society of the Pacific
462
232
No
No
International
1050-3390
San Francisco
CA
Progress in Solar/Stellar Physics with Helio- and Asteroseismology
13-17 Mars 2011
H. Shibahashi
Hakone
Japan
[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.
Researchers ; Professionals ; Students
http://hdl.handle.net/2268/164375

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