The 90-110 μm dust feature in low to intermediate mass protostars: Calcite?

Astronomy and Astrophysics

Volumn 432, Issue 2, 2005, Pages 547-557

  Chiavassa, A ^a   Ceccarelli, C ^a   Tielens, A G G M ^b   Caux, E ^c   Maret, S ^a  

^a LABORATOIRE D ASTROPHYSIQUE   (France)

^b UNIVERSITY OF GRONINGEN   (Netherlands)

^c IRAP   (France)

Author keywords

Infrared: ISM5; ISM: abundances; ISM: dust, extinction; ISM: lines and bands; ISM: molecules; Stars: formation

Indexed keywords

CARBONATES; MINERALOGY; MOLECULES; SILICATES; SPECTROSCOPIC ANALYSIS; SPECTRUM ANALYSIS; TELESCOPES;

ABUNDANCES-ISM; EXTINCTION-ISM; FAR INFRARED (FIR); FORMATION-ISM; ISM; LINES AND BANDS; MOLECULES-STARS;

ASTROPHYSICS;

EID: 15244353560     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041891     Document Type: Article

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