C i observations in the CQ Tauri proto-planetary disk: Evidence of a very low gas-to-dust ratio?

Astronomy and Astrophysics

Volumn 520, Issue 9, 2010, Pages

  Chapillon, E ^a   Parise, B ^a   Guilloteau, S ^b,c   Dutrey, A ^b,c   Wakelam, V ^b,c  

^a MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^b OBSERVATOIRE DE BORDEAUX   (France)

^c LABORATOIRE D ASTROPHYSIQUE DE BORDEAUX   (France)

Author keywords

circumstellar matter; protoplanetary disks; radio lines: stars; stars: individual: CQTau

Indexed keywords

CARBON CHEMISTRY; CHEMICAL MODEL; CIRCUMSTELLAR MATTERS; CLASS II; CO EMISSIONS; DEBRIS DISK; GAS CONTENT; PROTOPLANETARY DISKS; RADIO LINES: STARS; STARS: INDIVIDUAL: CQTAU; UPPER LIMITS; UV RADIATION;

DEBRIS; DISKS (MACHINE COMPONENTS); DUST; GASES; HIGH FREQUENCY TELECOMMUNICATION LINES; RADIO WAVES; STARS; ULTRAVIOLET RADIATION;

DISKS (STRUCTURAL COMPONENTS);

EID: 78349237028     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014841     Document Type: Article

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