Bulletin de la Société Royale des Sciences de Liège

0037-9565 1783-5720

 

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)
DOI: 10.25518/0037-9565.11266
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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 : http://popups.ulg.be/0037-9565/index.php?id=11266.

Over : M. D. Reed

Missouri State University, Springfield, MO, USA. Corresponding author: mikereed@missouristate.edu

Over : A. S. Baran

ARDASTELLA Research Group and Astronomical Observatory, University of Warsaw, Al. Ujazdowskie 4, 00-478 Warszawa, Poland

Over : R. H. Østensen

Recogito AS, Storgaten 72, N-8200 Fauske, Norway

Over : J. H. Telting

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

Over : C. S. Jeffery

Armagh Observatory and Planetarium, College Hill, Armagh BT61 9DG, N. Ireland