SIMBAD references

2018MNRAS.477..808L - Mon. Not. R. Astron. Soc., 477, 808-815 (2018/June-2)

Atmospheric mass-loss of extrasolar planets orbiting magnetically active host stars.

LALITHA S., SCHMITT J.H.M.M. and DASH S.

Abstract (from CDS):

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.

Abstract Copyright: © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): stars: activity - stars: coronae - stars: individual: (Kepler-63, Kepler-210, WASP-19, HAT-P-11) - stars: low-mass, late-type, planetary systems

Simbad objects: 17

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2021.06.25-09:04:28

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