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Massive star-formation toward G28.87+0.07

  • J. J. Li (a1) (a2), L. Moscadelli (a2), R. Cesaroni (a2), R. S. Furuya (a3), Y. Xu (a1), T. Usuda (a3), K. M. Menten (a4), M. Pestalozzi (a5), D. Eliav (a5) and E. Schisano (a5)...

Abstract

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.

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References

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Furuya, R. S., Cesaroni, R., Takahashi, S., et al. 2008, ApJ, 673, 363
Li, J. J., Moscadelli, L., Cesaroni, R., et al. 2012, ApJ, accepted
Moscadelli, L., Cesaroni, R., Rioja, M. J., et al. 2011, A&A, 526, 66
Sanna, A., Moscadelli, L., Cesaroni, R., et al. 2010a, A&A, 517, 71
Sanna, A., Moscadelli, L., Cesaroni, R., et al. 2010b, A&A, 517, 78
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