Evidence for pressure-driven flows and turbulent dissipation in the serpens NW cluster

Astrophysical Journal

Volumn 537, Issue 2 PART 1, 2000, Pages 891-903

  Williams, Jonathan P ^a,b   Myers, Philip C ^c  

^a NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

^b University of Florida ^*  (United States)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

ISM: individual (Serpens); ISM: kinematics and dynamics; Stars: formation; Turbulence

Indexed keywords

EID: 0034375711     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/309084     Document Type: Article

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