Turbulent flow-driven molecular cloud formation: A solution to the post-T Tauri problem?

Astrophysical Journal

Volumn 527, Issue 1 PART 1, 1999, Pages 285-297

  Ballesteros Paredes, Javier ^a,b   Hartmann, Lee ^b   Vázquez Semadeni, Enrique ^a  

^a UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

ISM: clouds; ISM: evolution; Stars: formation; Stars: pre main sequence; Turbulence

Indexed keywords

EID: 0000899810     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/308076     Document Type: Article

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