Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7275
Title: Atmospheric mass loss of extrasolar planets orbiting magnetically active host stars
Authors: Lalitha, Sairam
Schmitt, J. H. M. M
Dash, S
Keywords: Stars: activity;Stars: coronae;Stars: low-mass;Late-type;Planetary systems;Stars: individual: Kepler-63, Kepler-210, WASP-19, HAT-P-11
Issue Date: Jun-2018
Publisher: Oxford University Press on behalf of the Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, Vol. 477, No. 1, pp. 808–815
Abstract: Magnetic stellar activity of exoplanet hosts can lead to the production of large amounts of high-energy emission, which irradiates extrasolar planets, located in the immediate vicinity of such stars. This radiation is absorbed in the planets’ upper atmospheres, which consequently heat up and evaporate, possibly leading to an irradiation-induced mass-loss. We present a study of the high-energy emission in the four magnetically active planet-bearing host stars Kepler-63, Kepler-210, WASP-19, and HAT-P-11, based on new XMM-Newton observations. We find that the X-ray luminosities of these stars are rather high with orders of magnitude above the level of the active Sun. The total XUV irradiation of these planets is expected to be stronger than that of well studied hot Jupiters. Using the estimated XUV luminosities as the energy input to the planetary atmospheres, we obtain upper limits for the total mass loss in these hot Jupiters.
Description: Restricted Access
URI: http://hdl.handle.net/2248/7275
ISSN: 1365-2966
???metadata.dc.rights???: © Royal Astronomical Society
???metadata.dc.relation.uri???: https://doi.org/10.1093/mnras/sty732
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Atmospheric_mass_loss_of_extrasolar_planets_orbiting.pdfRestricted Access924.92 kBAdobe PDFView/Open    Request a copy


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.