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The distance to G59.7+0.1

Published online by Cambridge University Press:  01 March 2007

Y. Xu ,
M. J. Reid ,
K. M. Menten ,
A. Brunthaler ,
X. W. Zheng  and
L. Moscadelli
Y. Xu
Affiliation:
Max-Planck-Institute für Radioastronomie, Bonn, Germany email: xuye@mpifr-bonn.mpg.de Purple Mountain Observatory, Nanjing, China
M. J. Reid
Affiliation:
Harvard-Smithsonian Center for Astrophysics, USA
K. M. Menten
Affiliation:
Max-Planck-Institute für Radioastronomie, Bonn, Germany email: xuye@mpifr-bonn.mpg.de
A. Brunthaler
Affiliation:
Max-Planck-Institute für Radioastronomie, Bonn, Germany email: xuye@mpifr-bonn.mpg.de
X. W. Zheng
Affiliation:
Nanjing University, China
L. Moscadelli
Affiliation:
Arcetri Obs., Firenze, Italy
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Abstract

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We have measured the distance to the high-mass star-forming region G59.7+0.1, which harbors the far-infra-red source IRAS 19410+2336. The distance is 2.20 ± 0.11 kpc and was determined by triangulation using Very Long Baseline Array (VLBA) observations of 12.2 GHz methanol masers phase-referenced to two compact extragalactic radio sources.

Keywords

ISM: moleculesGalaxy: kinematics and dynamicsGalaxy: structure
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S242: Astrophysical Masers and their Environments , March 2007 , pp. 374 - 375
Copyright
Copyright © International Astronomical Union 2008

References

Beuther, H. & Schilke, P., 2004, Scince, 303, 1167CrossRefGoogle Scholar
Beuther, H. et al. 2002, A&A 390, 289Google Scholar
Xu, Y., Reid, M. J., X. W., , & Zheng, K. M. Menten 2006, Scince 311, 54Google Scholar