A review of seismic observations of Kepler and K2-Observed sdBV stars

This paper reviews recent seismic findings from Kepler and K2 data. Using three years of short cadence Kepler (K1) data, it is possible to examine time evolution of pulsations in an unprecedented way. While K2 observations are shorter, only three months, they are important as they are finding more s...

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Main Authors: Reed Michael D., Baran Andrzej S., Telting John H., Østensen Roy H., Jeffery Christopher S., Kern Joshua W., Ketzer Laura, Crooke John, Slayton A.
Format: Article
Language:English
Published: De Gruyter 2018-07-01
Series:Open Astronomy
Online Access:https://doi.org/10.1515/astro-2018-0015
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author Reed Michael D.
Baran Andrzej S.
Telting John H.
Østensen Roy H.
Jeffery Christopher S.
Kern Joshua W.
Ketzer Laura
Crooke John
Slayton A.
author_facet Reed Michael D.
Baran Andrzej S.
Telting John H.
Østensen Roy H.
Jeffery Christopher S.
Kern Joshua W.
Ketzer Laura
Crooke John
Slayton A.
author_sort Reed Michael D.
collection DOAJ
description This paper reviews recent seismic findings from Kepler and K2 data. Using three years of short cadence Kepler (K1) data, it is possible to examine time evolution of pulsations in an unprecedented way. While K2 observations are shorter, only three months, they are important as they are finding more sdBV stars than K1 did. Most importantly, K2 is discovering more p−mode pulsators with coverage not possible to get from the ground.
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spelling doaj.art-e80dde93682f457c80a3fc560a8961df2022-12-21T21:28:14ZengDe GruyterOpen Astronomy2543-63762018-07-0127115716610.1515/astro-2018-0015astro-2018-0015A review of seismic observations of Kepler and K2-Observed sdBV starsReed Michael D.0Baran Andrzej S.1Telting John H.2Østensen Roy H.3Jeffery Christopher S.4Kern Joshua W.5Ketzer Laura6Crooke John7Slayton A.8Department of Physics, Astronomy and Materials Science, Missouri StateUniversity, United States of AmericaDepartment of Physics, Astronomy and Materials Science, Missouri StateUniversity, United States of AmericaNordic Optical Telescope,Santa Cruz de Tenerife, SpainDepartment of Physics, Astronomy and Materials Science, Missouri StateUniversity, United States of AmericaArmagh Observatory and Planetarium,Armagh, IrelandDepartment of Physics, Astronomy and Materials Science, Missouri StateUniversity, United States of AmericaDepartment of Physics, Astronomy and Materials Science, Missouri StateUniversity, United States of AmericaDepartment of Physics, Astronomy and Materials Science, Missouri StateUniversity, United States of AmericaDepartment of Physics, Astronomy and Materials Science, Missouri StateUniversity, United States of AmericaThis paper reviews recent seismic findings from Kepler and K2 data. Using three years of short cadence Kepler (K1) data, it is possible to examine time evolution of pulsations in an unprecedented way. While K2 observations are shorter, only three months, they are important as they are finding more sdBV stars than K1 did. Most importantly, K2 is discovering more p−mode pulsators with coverage not possible to get from the ground.https://doi.org/10.1515/astro-2018-0015
spellingShingle Reed Michael D.
Baran Andrzej S.
Telting John H.
Østensen Roy H.
Jeffery Christopher S.
Kern Joshua W.
Ketzer Laura
Crooke John
Slayton A.
A review of seismic observations of Kepler and K2-Observed sdBV stars
Open Astronomy
title A review of seismic observations of Kepler and K2-Observed sdBV stars
title_full A review of seismic observations of Kepler and K2-Observed sdBV stars
title_fullStr A review of seismic observations of Kepler and K2-Observed sdBV stars
title_full_unstemmed A review of seismic observations of Kepler and K2-Observed sdBV stars
title_short A review of seismic observations of Kepler and K2-Observed sdBV stars
title_sort review of seismic observations of kepler and k2 observed sdbv stars
url https://doi.org/10.1515/astro-2018-0015
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