Trigonometric parallaxes of massive star-forming regions. VII. G9.62+0.20 and the expanding 3 kpc ARM

Astrophysical Journal

Volumn 706, Issue 1, 2009, Pages 464-470

  Sanna, A ^a,b,c   Reid, M J ^c   Moscadelli, L ^d   Dame, T M ^c   Menten, K M ^e   Brunthaler, A ^e   Zheng, X W ^f   Xu, Y ^g  

^a UNIVERSITY OF CAGLIARI   (Italy)

^b INAF OSSERVATORIO ASTRONOMICO DI CAGLIARI   (Italy)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^e MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^f NANJING UNIVERSITY   (China)

^g CHINESE ACADEMY OF SCIENCES   (China)

Author keywords

Astrochemistry; Galaxy: Fundamental parameters; Galaxy: Kinematics and dynamics; Masers; Stars: Formation; Techniques: High angular resolution

Indexed keywords

EID: 70549098999     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/706/1/464     Document Type: Article

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