Kepler, K2, and TESS observations: ensemble and comparative asteroseismology

Authors

• Michael D. Reed, Missouri State UniversityFollow
• Andrzej S. Baran, Missouri State UniversityFollow
• Østensen, Recogito AS
• Telting, Aarhus Universitet
• Jeffery, Armagh Observatory

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.

Department(s)

Physics, Astronomy, and Materials Science

Document Type

Article

DOI

10.255118/0037-9565.11266

Publication Date

1-1-2023

Recommended Citation

Reed, Michael D.; Baran, Andrzej S.; Østensen; Telting; and Jeffery, "Kepler, K2, and TESS observations: ensemble and comparative asteroseismology" (2023). Faculty Scholarship. 694.
https://bearworks.missouristate.edu/articles00/694

Journal Title

Bulletin De La Societe Royale Des Sciences De Liege