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Stellar winds from hot low-mass stars

✍ Scribed by W.-R. Hamann

Publisher
Springer Netherlands
Year
2010
Tongue
English
Weight
584 KB
Volume
329
Category
Article
ISSN
0004-640X

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We present an analytic model for the interaction between planetary atmospheres and stellar winds from main sequence M stars, with the purpose of obtaining a quick test-model that estimates the timescale for total atmospheric mass loss due to this interaction. Planets in the habitable zone of M dwarf