M dwarfs: planet formation and long term evolution

The first part of this paper discusses how planet formation proceeds in the disks orbiting M dwarf stars. These environments are different from those associated with solar‐type stars in several ways: The planet forming clock (set by orbits) runs slower, the disks are more prone to evaporation, the s...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	Astronomische Nachrichten 2005-12, Vol.326 (10), p.913-919
Hauptverfasser:	Adams, F. C., Bodenheimer, P., Laughlin, G.
Format:	Artikel
Sprache:	eng
Schlagworte:	evolution planets: formation protoplanetary disks red giants stars: formation stars: formation, evolution stars: late-type (M dwarfs stars: late‐type (M dwarfs, red giants)
Online-Zugang:	Volltext
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