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- Kepler, K2, and TESS observations: ensemble and comparative asteroseismology
sinds 05 februari 2011 :
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M. D.
Reed, A. S.
Baran, R. H.
Østensen, J. H.
Telting & C. S.
Jeffery Kepler, K2, and TESS observations: ensemble and comparative asteroseismology
(Volume 92 - Année 2023 — Numéro 2 - Proceedings of the 10th Meeting on Hot Subdwarfs and Related Objects)
Article
Abstract
The original Kepler mission detected 18 pulsating subdwarf B (sdBV) stars, K2 observed 161 of our proposed targets with 41 sdB stars found to show p- or g-mode pulsations, and TESS has observed about 1,000 of our proposed targets. All these data should provide ∼300 sdBV stars, from which asteroseismology will provide a host of measurables. Combined with temperatures and gravities (and radii and masses from GAIA parallaxes!), we have a powerful set of observations with which to compare models. Here we review our seismology progress with sdBV stars.
Om dit artikel te citeren:
M. D. Reed, A. S. Baran, R. H. Østensen, J. H. Telting & C. S. Jeffery, «Kepler, K2, and TESS observations: ensemble and comparative asteroseismology», Bulletin de la Société Royale des Sciences de Liège [En ligne], Volume 92 - Année 2023, Numéro 2 - Proceedings of the 10th Meeting on Hot Subdwarfs and Related Objects, 81-93 URL : https://popups.uliege.be/0037-9565/index.php?id=11266.
ARDASTELLA Research Group and Astronomical Observatory, University of Warsaw, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
Recogito AS, Storgaten 72, N-8200 Fauske, Norway
Nordic Optical Telescope, Rambla José Ana Fernández Pérez 7, 38711 Breña Baja, Spain and Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark
Armagh Observatory and Planetarium, College Hill, Armagh BT61 9DG, N. Ireland