Activity and differential rotation of the early M dwarf Kepler-45 from transit mapping
dc.contributor.author | Zaleski S.M. | |
dc.contributor.author | Valio A. | |
dc.contributor.author | Carter B.D. | |
dc.contributor.author | Marsden S.C. | |
dc.date.accessioned | 2024-03-12T23:48:35Z | |
dc.date.available | 2024-03-12T23:48:35Z | |
dc.date.issued | 2020 | |
dc.description.abstract | © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society.Little is known of the activity and differential rotation of low luminosity, early M dwarfs from direct observation. We present the first stellar activity analysis of star-spots and faculae for the hot Jupiter hosting M1V dwarf Kepler-45 from Kepler transit light curves. We find star-spot and facula temperatures contrasting a few hundred degrees with the quiet photosphere, hence similar to other early M dwarfs having a convective envelope surrounding a radiative core. Star-spots are prominent close to the centre of the stellar disc, with faculae prominent towards the limbs, similar to what is observed for the Sun. Star-spot and facula mean sizes are about 40 and 45 × 103 km, respectively, and thus faculae occupy a 10 per cent larger surface area than the star-spots. A short-term activity cycle of about 295 d is observed that is reminiscent of those seen for other cool dwarfs. Adopting a solar-type differential rotation profile (faster equatorial rotation than polar rotation), our star-spot and facula temporal mapping indicates a rotation period of 15.520 ± 0.025 d at the transit latitude of -33.2°. From the mean stellar rotation of 15.762 d, we estimate a rotational shear of 0.031 ± 0.004 rad d-1, or a relative differential rotation of 7.8 ± 0.9 per cent. Kepler-45's surface rotational shear is thus consistent with observations and theoretical modelling of other early M dwarfs that indicate a shear of less than 0.045 rad d-1 and no less than 0.03 rad d-1 for stars with similar stellar rotation periods. | |
dc.description.firstpage | 5141 | |
dc.description.issuenumber | 4 | |
dc.description.lastpage | 5151 | |
dc.description.volume | 492 | |
dc.identifier.doi | 10.1093/mnras/staa103 | |
dc.identifier.issn | 1365-2966 | |
dc.identifier.uri | https://dspace.mackenzie.br/handle/10899/35014 | |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
dc.rights | Acesso Aberto | |
dc.subject.otherlanguage | stars: activity | |
dc.subject.otherlanguage | stars: solar-type | |
dc.subject.otherlanguage | starspots | |
dc.title | Activity and differential rotation of the early M dwarf Kepler-45 from transit mapping | |
dc.type | Artigo | |
local.scopus.citations | 10 | |
local.scopus.eid | 2-s2.0-85100307932 | |
local.scopus.subject | Differential rotation | |
local.scopus.subject | Direct observations | |
local.scopus.subject | Rotation period | |
local.scopus.subject | Rotational shear | |
local.scopus.subject | Star spots | |
local.scopus.subject | Star: activity | |
local.scopus.subject | Stars: solar types | |
local.scopus.subject | Starspots | |
local.scopus.subject | Stellar rotation | |
local.scopus.subject | Stellars | |
local.scopus.updated | 2024-05-01 | |
local.scopus.url | https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85100307932&origin=inward |