Physical and chemical conditions in methanol maser selected hot cores and UCH ii regions

Monthly Notices of the Royal Astronomical Society

Volumn 394, Issue 1, 2009, Pages 323-339

  Purcell, C R ^a,b   Longmore, S N ^b,c,d   Burton, M G ^b   Walsh, A J ^b,e   Minier, V ^b,f   Cunningham, M R ^b   Balasubramanyam, R ^b,g  

^a UNIVERSITY OF MANCHESTER   (United Kingdom)

^b UNIVERSITY OF NEW SOUTH WALES   (Australia)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d CSIRO   (Australia)

^e JAMES COOK UNIVERSITY   (Australia)

^f UNIVERSITÉ PARIS DIDEROT   (France)

^g RAMAN RESEARCH INSTITUTE   (India)

Author keywords

ISM: abundances; ISM: molecules; Stars: formation; Stars: pre main sequence; Surveys

Indexed keywords

ANTENNAS; INDICATORS (CHEMICAL); MASERS; METHANOL; STARS;

CHEMICAL CONDITIONS; ISM: ABUNDANCE; ISM:MOLECULES; MEASUREMENTS OF; METHANOL MASERS; PHYSICAL CONDITIONS; RADIO EMISSION; SPECTRAL LINE SURVEY; STARS FORMATION; STARS: PRE-MAIN SEQUENCE;

SURVEYS;

EID: 62349112547     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.14283.x     Document Type: Article

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