Modeling of the dust and gas outflows from OH 26.5 + 0.6: The superwind

Astrophysical Journal

Volumn 456, Issue 1 PART I, 1996, Pages 337-349

  Justtanont, K ^a,g   Skinner, C J ^b,f   Tielens, A G G M ^c   Meixner, M ^d   Baas, F ^e  

^a NASA AMES RESEARCH CENTER   (United States)

^b INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^c AURA for the European Space Agency   (United States)

^d LAWRENCE LIVERMORE NATIONAL LABORATORY   (United States)

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

^f LEIDEN UNIVERSITY   (Netherlands)

^g UNIVERSITY OF HAWAII   (United States)

Author keywords

Circumstellar matter; Dust, extinction; Infrared: Stars; Stars: Agb and post agb; Stars: Mass loss

Indexed keywords

EID: 21844504007     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/176655     Document Type: Article

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