The high-velocity molecular stream in W51B: A ring structure with compact H II regions

Monthly Notices of the Royal Astronomical Society

Volumn 296, Issue 4, 1998, Pages 863-868

  Moon, D S ^a   Park, Y S ^b  

^a Seoul National University   (South Korea)

^b Korea Astronomy and Space Science Institute (KASI)   (South Korea)

Author keywords

H II regions; ISM: clouds; ISM: individual: W51B; ISM: molecules; Radio lines: ISM

Indexed keywords

KINETIC ENERGY; KINETICS; MASS SPECTROMETRY; VELOCITY;

H II REGIONS; HIGH VELOCITY; ISM : CLOUDS; ISM: INDIVIDUAL: W51B; ISM: INDIVIDUALS; ISM:MOLECULES; MAXIMUM VELOCITY; MOLECULAR GAS; RADIO LINES: ISM; RINGS STRUCTURE;

MOLECULES;

EID: 0040983205     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01423.x     Document Type: Article

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