The characteristics of the IR emission features in the spectra of Herbig Ae stars: Evidence for chemical evolution

Astronomy and Astrophysics

Volumn 484, Issue 1, 2008, Pages 241-249

  Boersma, C ^a   Bouwman, J ^b   Lahuis, F ^c,d   Van Kerckhoven, C ^e   Tielens, M ^a,f   Waters, M ^g   Henning, T ^b  

^a UNIVERSITY OF GRONINGEN   (Netherlands)

^b MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^c SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

^d LEIDEN UNIVERSITY   (Netherlands)

^e KU LEUVEN   (Belgium)

^f NASA AMES RESEARCH CENTER   (United States)

^g UNIVERSITY OF AMSTERDAM   (Netherlands)

Author keywords

Infrared: stars; ISM: molecules; Line: profiles; Stars: planetary systems: formation

Indexed keywords

ASTROPHYSICS; GALAXIES; INFRARED SPECTROGRAPHS; POLYCYCLIC AROMATIC HYDROCARBONS; SPACE TELESCOPES;

INFRARED: STARS; PLANETARY SYSTEMS; STAR FORMATION;

STARS;

EID: 44349101951     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078001     Document Type: Article

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