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Massive star-formation toward G28.87+0.07

Published online by Cambridge University Press:  24 July 2012

J. J. Li ,
L. Moscadelli ,
R. Cesaroni ,
R. S. Furuya ,
Y. Xu ,
T. Usuda ,
K. M. Menten ,
M. Pestalozzi ,
D. Eliav  and
E. Schisano
J. J. Li
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, email: jjli@pmo.ac.cn INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy
L. Moscadelli
Affiliation:
INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy
R. Cesaroni
Affiliation:
INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy
R. S. Furuya
Affiliation:
Subaru Telescope, National Astronomical Observatory of Japan, 650 North A'ohoku Place, Hilo, HI 96720, USA
Y. Xu
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, email: jjli@pmo.ac.cn
T. Usuda
Affiliation:
Subaru Telescope, National Astronomical Observatory of Japan, 650 North A'ohoku Place, Hilo, HI 96720, USA
K. M. Menten
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
M. Pestalozzi
Affiliation:
INAF-Istituto Fisica Spazio Interplanetario, Via Fosso del Cavaliere 100, I-00133 Roma, Italy
D. Eliav
Affiliation:
INAF-Istituto Fisica Spazio Interplanetario, Via Fosso del Cavaliere 100, I-00133 Roma, Italy
E. Schisano
Affiliation:
INAF-Istituto Fisica Spazio Interplanetario, Via Fosso del Cavaliere 100, I-00133 Roma, Italy
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Abstract

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We investigated the high-mass star-forming region G28.87+0.07 by means of maser kinematics, including H2O, CH3OH, and OH, and radio to infrared, continuum observations. All observational evidence suggests that these masers are associated with the same young star of 20-30 M⊙, still in the main accretion phase and surrounded by a rich stellar cluster.

Keywords

ISM: individual objects (G28.87+0.07) – ISM: kinematics and dynamics – masers – techniques: interferometric
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S287: Cosmic Masers - from OH to H0 , January 2012 , pp. 180 - 181
Copyright
Copyright © International Astronomical Union 2012

References

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Li, J. J., Moscadelli, L., Cesaroni, R., et al. 2012, ApJ, acceptedGoogle Scholar
Moscadelli, L., Cesaroni, R., Rioja, M. J., et al. 2011, A&A, 526, 66Google Scholar
Sanna, A., Moscadelli, L., Cesaroni, R., et al. 2010a, A&A, 517, 71Google Scholar
Sanna, A., Moscadelli, L., Cesaroni, R., et al. 2010b, A&A, 517, 78Google Scholar