Are aspherical AGB shells due to aspherical central stars?

Astronomy and Astrophysics

Volumn 305, Issue 3, 1996, Pages

  Groenewegen, M A T ^a,b,c  

^a CNRS   (France)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^c MPA ^*

Author keywords

Circumstellar matter; Stars: AGB, post AGB; Stars: individual: IRC +10 216; Stars: mass loss

Indexed keywords

EID: 0010202080     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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