The hydrodynamic evolution of circumstellar gas around massive stars: II. The impact of the time sequence O star → RSG → WR star

Astronomy and Astrophysics

Volumn 316, Issue 1, 1996, Pages 133-146

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

^a UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

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

^c INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^d MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^e UNIVERSITY OF CHICAGO   (United States)

^f MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

Author keywords

Hydrodynamics; ISM: bubbles; Stars: evolution; Stars: mass loss; Stars: Wolf Rayet; supergiants

Indexed keywords

EID: 0000907734     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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