Theoretical models of the planetary nebula populations in galaxies: The ISM oxygen abundance when star formation stops

Astronomy and Astrophysics Supplement Series

Volumn 122, Issue 2, 1997, Pages 215-233

  Richer, M G ^a   McCall, M L ^b   Arimoto, N ^c  

^a OBSERVATOIRE DE PARIS   (France)

^b YORK UNIVERSITY   (Canada)

^c UNIVERSITY OF TOKYO   (Japan)

Author keywords

Galaxies: abundances, evolution, stellar content; ISM: planetary nebulae: general; Stars: AGB and post AGB

Indexed keywords

EID: 3643139091     PISSN: 03650138     EISSN: None     Source Type: Journal    
DOI: 10.1051/aas:1997131     Document Type: Article

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