Reference : g-Mode Oscillations in Hot B Subdwarf Stars
Scientific congresses and symposiums : Paper published in a journal
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/161250
g-Mode Oscillations in Hot B Subdwarf Stars
English
Charpinet, Stéphane []
Van Grootel, Valérie mailto [Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie >]
Fontaine, Gilles []
Brassard, Pierre []
Green, Elizabeth M []
Randall, Suzanna K []
Dec-2013
Astronomical Society of the Pacific Conference Series
Astronomical Society of the Pacific
479
Progress in Physics of the Sun and Stars: A New Era in Helio- and Asteroseismology
263
Yes
Yes
International
1050-3390
San Francisco
CA
Fujihara Seminar 2012
25 au 30 novembre 2012
H. Shibahashi
Hakone
Japan
[en] Observations from space with CoRoT and Kepler have revealed the rich pulsation spectra that characterize the long period hot B subdwarf (sdB) pulsators of the V1093 Her type. These evolved and compact helium core burning stars can develop low amplitude oscillations with periods in the range ∼ 1 − 4 hours that correspond to low degree, mid to high order g-modes. These modes have the property to penetrate deep inside the star, down to the boundary of the central convective core. They are consequently particularly interesting as asteroseismic probes. Here we briefly review how the g-modes behave in sdB stars, focusing in particular on the seismic signatures coming from the core itself. We also briefly summarize the first seismic results obtained from space data in pioneering efforts to exploit the potential of long period sdB pulsators as deep probes of the core structure.
Researchers ; Professionals ; Students
http://hdl.handle.net/2268/161250

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