Erratum: The Ortho-to-Para Ratio and the Chemical Properties of C3H2 in Dark Cloud Cores (Publications of the Astronomical Society of Japan (2001) 53 (251–257) DOI: 10.1093/pasj/53.2.251);The ortho-to-para ratio and the chemical properties of C3H2 in dark cloud cores

Publications of the Astronomical Society of Japan

Volumn 53, Issue 2, 2001, Pages 251-257

  Takakuwa, Shigehisa ^a,c   Kawaguchi, Kentarou ^a,d   Mikami, Hitomi ^a   Saito, Masao ^b  

^a NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c INSTITUTE OF ASTRONOMY AND ASTROPHYSICS   (Taiwan)

^d OKAYAMA UNIVERSITY   (Japan)

Author keywords

ISM: abundances; ISM: individual (TMC 1C, L 1527); ISM: molecules

Indexed keywords

MOLECULES; STARS;

DUST TEMPERATURES; EQUILIBRIUM ANALYSIS; ISM: ABUNDANCE; ISM: INDIVIDUAL (TMC-1C, L 1527); ISM: INDIVIDUALS; ISM:MOLECULES; PRECURSOR MOLECULES; STATISTICAL EQUILIBRIUM; THERMAL-EQUILIBRIUM; WAVELENGTH REGIONS;

MILLIMETER WAVES;

EID: 0035633778     PISSN: 00046264     EISSN: 2053051X     Source Type: Journal    
DOI: 10.1093/pasj/53.3.577     Document Type: Erratum

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