Atmospheric mass loss by stellar wind from planets around main sequence M stars

@article{Zendejas2010AtmosphericML,
  title={Atmospheric mass loss by stellar wind from planets around main sequence M stars},
  author={Jesus Zendejas and Ant'igona Segura and Alejandro Raga},
  journal={Icarus},
  year={2010},
  volume={210},
  pages={539-544}
}
Abstract 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 dwarfs may be tidally locked and may have weak magnetic fields, because of this we consider the extreme case of planets with no magnetic field. The model gives the planetary atmosphere mass loss… Expand

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