SIMBAD references

2019MNRAS.489..437D - Mon. Not. R. Astron. Soc., 489, 437-445 (2019/October-2)

Probing the origin of stellar flares on M dwarfs using TESS data sectors 1-3.

DOYLE L., RAMSAY G., DOYLE J.G. and WU K.

Abstract (from CDS):

Detailed studies of the Sun have shown that sunspots and solar flares are closely correlated. Photometric data from Kepler/K2 has allowed similar studies to be carried out on other stars. Here, we utilize Transiting Exoplanet Survey Satellite (TESS) photometric 2-min cadence of 167 low-mass stars from Sectors 1 to 3 to investigate the relationship between star-spots and stellar flares. From our sample, 90 per cent show clear rotational modulation likely due to the presence of a large, dominant star-spot and we use this to determine a rotational period for each star. Additionally, each low-mass star shows one or more flares in its light curve and using Gaia Data Release 2 parallaxes and SkyMapper magnitudes we can estimate the energy of the flares in the TESS band-pass. Overall, we have 1834 flares from the 167 low-mass stars with energies from 6.0 x 1029 to 2.4 x 1035 erg. We find none of the stars in our sample show any preference for rotational phase, suggesting the lack of a correlation between the large, dominant star-spot, and flare number. We discuss this finding in greater detail and present further scenarios to account for the origin of flares on these low-mass stars.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): stars: activity - stars: flare - stars: low-mass - stars: magnetic fields

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.

Simbad objects: 13

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2021.06.20-04:54:52

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