A new derivation of the extinction-to-CO column density ratio in the Chamaeleon I dark cloud

Publications of the Astronomical Society of Japan

Volumn 51, Issue 6, 1999, Pages 919-929

  Hayakawa, Takahiro ^a   Mizuno, Akira ^a   Onishi, Toshikazu ^a   Yonekura, Yoshinori ^b   Hara, Atsushi ^a   Yamaguchi, Reiko ^a   Fukui, Yasuo ^a  

^a NAGOYA UNIVERSITY   (Japan)

^b Osaka Prefecture University   (Japan)

Author keywords

ISM: clouds; ISM: dust, extinction; ISM: individual (Chamaeleon I); ISM: molecules

Indexed keywords

COLUMN DENSITY; DENSITY RATIO; DUST EXTINCTIONS; ISM : CLOUDS; ISM: DUST, EXTINCTION; ISM: INDIVIDUAL (CHAMELEON I); ISM: INDIVIDUALS; ISM:DUST; ISM:MOLECULES; T TAURI STARS;

STARS;

EID: 0033236534     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/51.6.919     Document Type: Article

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