Spots and Flares in Hot Main Sequence Stars Observed by Kepler, K2, and TESS

About 22,000 Kepler stars, 7,000 K2 stars, and nearly 60,000 TESS stars from sectors 1–24 have been classified according to variability type. A large proportion of stars of all spectral types appear to have periods in their light curves consistent with the expected rotation periods. A previous analy...

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Main Author: Luis A. Balona
Format: Article
Language:English
Published: Frontiers Media S.A. 2021-03-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
Online Access:https://www.frontiersin.org/articles/10.3389/fspas.2021.580907/full
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author Luis A. Balona
author_facet Luis A. Balona
author_sort Luis A. Balona
collection DOAJ
description About 22,000 Kepler stars, 7,000 K2 stars, and nearly 60,000 TESS stars from sectors 1–24 have been classified according to variability type. A large proportion of stars of all spectral types appear to have periods in their light curves consistent with the expected rotation periods. A previous analysis of A- and late B-type stars suggests that these stars are indeed rotational variables. In this paper we have accumulated data to show that rotational modulation is present in about 30–40% of A- and B-type stars. A search for flares in TESS A- and B-type stars resulted in the detection of 102 flares in 57 stars. Analysis of flare energies show that the source of the flares cannot be a cool dwarf companion nor a F/G giant. The realization that a considerable fraction of A- and B-type stars are active indicates that a revision of current concepts regarding hot star envelopes is required.
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spelling doaj.art-1b389247928d4b65a9ee3b1ea17a00a62022-12-21T22:24:42ZengFrontiers Media S.A.Frontiers in Astronomy and Space Sciences2296-987X2021-03-01810.3389/fspas.2021.580907580907Spots and Flares in Hot Main Sequence Stars Observed by Kepler, K2, and TESSLuis A. BalonaAbout 22,000 Kepler stars, 7,000 K2 stars, and nearly 60,000 TESS stars from sectors 1–24 have been classified according to variability type. A large proportion of stars of all spectral types appear to have periods in their light curves consistent with the expected rotation periods. A previous analysis of A- and late B-type stars suggests that these stars are indeed rotational variables. In this paper we have accumulated data to show that rotational modulation is present in about 30–40% of A- and B-type stars. A search for flares in TESS A- and B-type stars resulted in the detection of 102 flares in 57 stars. Analysis of flare energies show that the source of the flares cannot be a cool dwarf companion nor a F/G giant. The realization that a considerable fraction of A- and B-type stars are active indicates that a revision of current concepts regarding hot star envelopes is required.https://www.frontiersin.org/articles/10.3389/fspas.2021.580907/fullstellar activitystellar rotationstar spotsflare starstime series
spellingShingle Luis A. Balona
Spots and Flares in Hot Main Sequence Stars Observed by Kepler, K2, and TESS
Frontiers in Astronomy and Space Sciences
stellar activity
stellar rotation
star spots
flare stars
time series
title Spots and Flares in Hot Main Sequence Stars Observed by Kepler, K2, and TESS
title_full Spots and Flares in Hot Main Sequence Stars Observed by Kepler, K2, and TESS
title_fullStr Spots and Flares in Hot Main Sequence Stars Observed by Kepler, K2, and TESS
title_full_unstemmed Spots and Flares in Hot Main Sequence Stars Observed by Kepler, K2, and TESS
title_short Spots and Flares in Hot Main Sequence Stars Observed by Kepler, K2, and TESS
title_sort spots and flares in hot main sequence stars observed by kepler k2 and tess
topic stellar activity
stellar rotation
star spots
flare stars
time series
url https://www.frontiersin.org/articles/10.3389/fspas.2021.580907/full
work_keys_str_mv AT luisabalona spotsandflaresinhotmainsequencestarsobservedbykeplerk2andtess