Resolving distance ambiguities towards 6.7 GHz methanol masers

Astronomy and Astrophysics

Volumn 486, Issue 1, 2008, Pages 191-208

  Pandian, J D ^a   Momjian, E ^b,d   Goldsmith, P F ^c  

^a MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^b Arecibo Observatory   (Puerto Rico)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

Author keywords

Galaxy: kinematics and dynamics; Galaxy: structure; H II regions

Indexed keywords

ABSORPTION; ELECTROMAGNETISM; GALAXIES; KINEMATICS; LEAD; MAGNETISM; MASERS; METHANOL; MICROWAVE AMPLIFIERS; SEMANTICS;

(P ,P ,T) MEASUREMENTS; DIFFERENTIAL ROTATION; EARLY STAGES; LARGE ARRAYS; MAXIMUM VELOCITY; METHANOL MASERS; RADIAL VELOCITY (RV); SPECTRA (CO); STAR FORMING COMPLEXES; STAR-FORMING REGIONS; TANGENT POINT;

SPEED;

EID: 46649096032     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809799     Document Type: Article

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