Water maser motions in W3(OH) and a determination of its distance

Astrophysical Journal

Volumn 645, Issue 1 I, 2006, Pages 337-344

  Hachisuka, K ^a,b   Brunthaler, A ^a,c   Menten, K M ^a   Reid, M J ^d   Imai, H ^e   Hagiwara, Y ^f,g   Mlyoshl, M ^f   Horiuchi, S ^h   Sasao, T ⁱ  

^a MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^b UNIVERSITY OF VALENCIA   (Spain)

^c JOINT INSTITUTE FOR VLBI IN EUROPE   (Netherlands)

^d HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^e KAGOSHIMA UNIVERSITY   (Japan)

^f NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^g ASTRON   (Netherlands)

^h SWINBURNE UNIVERSITY OF TECHNOLOGY   (Australia)

ⁱ Ajou University   (South Korea)

Author keywords

Astrometry; Masers; Stars: distances; Stars: formation; Stars: individual (W3(OH)); Stellar dynamics

Indexed keywords

EID: 33746904726     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/502962     Document Type: Article

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