Modelling enhanced density shells in the circumstellar envelope of IRC +10216

Monthly Notices of the Royal Astronomical Society

Volumn 339, Issue 4, 2003, Pages 1041-1047

  Brown, J M ^a,c   Millar, T J ^b  

^a SWARTHMORE COLLEGE   (United States)

^b UNIVERSITY OF MANCHESTER   (United Kingdom)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

Circumstellar matter; Ism: Molecules; Molecular data; Molecular processes; Stars: Individual: Irc +10216

Indexed keywords

CARBON; MOLECULAR STRUCTURE; MOLECULES; SHELLS (STRUCTURES);

ASYMPTOTIC GIANT BRANCH STARS; CARBON STARS; CIRCUMSTELLAR ENVELOPES; CIRCUMSTELLAR MATTERS; ISM:MOLECULES; LATE-TYPE; MOLECULAR DATA; MOLECULAR PROCESS; STAR: INDIVIDUAL: IRC +10216; STARS: INDIVIDUAL: PROXIMA CENTAURI;

STARS;

EID: 0142073859     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06252.x     Document Type: Article

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