Physical conditions in the proto-planetary nebula CRL 618 derived from observations of vibrationally excited HC3N

Astrophysical Journal

Volumn 586, Issue 1 I, 2003, Pages 344-355

  Wyrowski, F ^a,b   Schilke, P ^b   Thorwirth, S ^c   Menten, K M ^b   Winnewisser, G ^c  

^a University of Maryland   (United States)

^b MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^c UNIVERSITY OF COLOGNE   (Germany)

Author keywords

Circumstellar matter; Line: profiles; Radio lines: stars; Stars: AGB and post AGB; Stars: individual (CRL 618); Stars: mass loss

Indexed keywords

EID: 0042134576     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/367637     Document Type: Article

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