SIMBAD references

2004ApJ...602L..53I - Astrophys. J., 602, L53-L56 (2004/February-2)

On the star-magnetosphere interaction of close-in exoplanets.

IP W.-H., KOPP A. and HU J.-H.

Abstract (from CDS):

Numerical simulations using a resistive MHD code are performed in order to investigate the interaction of the magnetospheres of hot Jupiters (or close-in extrasolar giant planets) with the central host stars. Because of the sub-Alfvénic nature of the stellar wind outflow at the orbital positions of these close-in exoplanets, no bow shock would form. When the orientation of the stellar coronal magnetic field is favorable to strong coupling with magnetic reconnection, the power (∼1027 ergs/s) generated could reach the level of a typical solar flare. As a particular type of star-planet atmospheric interaction, as investigated by Cuntz, Saar, & Musielak, magnetospheric interaction as studied in this Letter could lead to extensive energy injection into the auroral zones of the exoplanets, producing massive atmospheric escape process as recently detected.

Abstract Copyright:

Journal keyword(s): Magnetic Fields - Stars: Planetary Systems - Stars: Atmospheres - Stars: Chromospheres - Stars: Flare

Simbad objects: 10

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2019.10.21-03:17:29

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