The dynamical evolution of circumstellar gas around massive stars I. The impact of the time sequence O star → LBV → WR star

Astronomy and Astrophysics

Volumn 305, Issue 1, 1996, Pages 229-244

  García Segura, Guillermo ^a,b,e   Mac Low, Mordecai Mark ^a,c   Langer, Norbert ^d  

^a UNIVERSITY OF ILLINOIS AT URBANA CHAMPAIGN   (United States)

^b INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^c UNIVERSITY OF CHICAGO   (United States)

^d MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^e UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

Author keywords

Hydrodynamics ; ISM: bubbles; ISM: individual (RCW 58); Stars: evolution, mass loss; Stars: Wolf Rayet

Indexed keywords

EID: 0000292579     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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