The shape and strength of circumstellar PAH emission bands

Astronomy and Astrophysics

Volumn 315, Issue 2, 1996, Pages

  Molster, F J ^a   Van Den Ancker, M E ^a   Tielens, A G G M ^b   Waters, L B F M ^a,c   Beintema, D A ^c   Waelkens, C ^d   De Jong, T ^a,c   De Graauw, Th ^c   Justtanont, K ^c   Yamamura, I ^c   Vandenbussche, B ^d,e   Heras, A ^e  

^a UNIVERSITY OF AMSTERDAM   (Netherlands)

^b NASA AMES RESEARCH CENTER   (United States)

^c SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

^d KU LEUVEN   (Belgium)

^e EUROPEAN SPACE AGENCY   (Spain)

Author keywords

Dust; Infrared: stars; Planetary nebulae; Stars: AGB and post AGB; Stars: mass loss

Indexed keywords

EID: 3342999477     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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