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arXiv · 1101.1913

Planet Formation Around M-dwarfs: From Young Disks to Planets

I. Pascucci·G. Laughlin·B. S. Gaudi·G. Kennedy·K. Luhman·S. Mohanty·J. Birkby·B. Ercolano·P. Plavchan·A. Skemer
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Abstract

Cool M dwarfs outnumber sun-like G stars by ten to one in the solar neighborhood. Due to their proximity, small size, and low mass, M-dwarf stars are becoming attractive targets for exoplanet searches via almost all current search methods. But what planetary systems can form around M dwarfs? Following up on the Cool Stars~16 Splinter Session "Planet Formation Around M Dwarfs", we summarize here our knowledge of protoplanetary disks around cool stars, how they disperse, what planetary systems might form and can be detected with current and future instruments.

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I. Pascucci, G. Laughlin, B. S. Gaudi, G. Kennedy, K. Luhman, S. Mohanty, J. Birkby, B. Ercolano, P. Plavchan, A. Skemer. 2011-01-10. Planet Formation Around M-dwarfs: From Young Disks to Planets. https://arxiv.org/abs/1101.1913

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