Exoplanets as probes of the winds of host stars: the case of the M dwarf GJ 436
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DOI: 10.1093/mnras/stx1543
Abstract: Winds of cool dwarfs are difficult to observe, with only a few M dwarfs presenting observationally-derived mass-loss rates (Mdot), which span several orders of magnitude. Close-in exoplanets are conveniently positioned in the inner regions of… read more here.
Keywords: stellar wind; wind; exoplanets probes; host stars ... See more keywords