Hostname: page-component-78c5997874-8bhkd Total loading time: 0 Render date: 2024-11-10T10:14:46.636Z Has data issue: false hasContentIssue false
  • English
  • Français

Methanol masers in the Herschel era Putting them in the star formation context

Published online by Cambridge University Press:  24 July 2012

Michele Pestalozzi
Michele Pestalozzi*
Affiliation:
IAPS - INAF, via del Fosso del Cavaliere 100, 00133 Roma, Italy email: michele.pestalozzi@gmail.com
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Methanol masers are known to be among the most reliable tracers of high-mass stars in early stages of evolution. A number of searches across the Galaxy has yielded to date, a complete census of those masers in two thirds of the Milky Way, providing a catalogue of some 800 sources to be studied in depth. In particular, it is important to characterise the physical properties of the objects hosting methanol masers, and this is possible today using data from the Herschel Space Observatory (HSO). The exceptional spatial resolution of HSO and its wavelength coverage are perfectly tuned to put the methanol maser phase into its star formation context. This paper presents results on the characterisation of methanol maser hosts using Herschel data from the Hi-GAL project, an Open Time Key Project to survey the inner Galactic plane at 5 wavelengths between 70 and 500 μm.

Keywords

Star formationhigh-mass starsmasersmethanol
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S287: Cosmic Masers - from OH to H0 , January 2012 , pp. 492 - 496
Copyright
Copyright © International Astronomical Union 2012

References

Caswell, J. L., Fuller, G. A., Green, J. A., et al. 2011, MNRAS, 1330Google Scholar
Ellingsen, S. P. 2006, ApJ, 638, 241CrossRefGoogle Scholar
Green, J. A., Caswell, J. L., Fuller, G. A., et al. 2008, MNRAS, 385, 948CrossRefGoogle Scholar
Griffin, M. J., Abergel, A., Abreu, A., et al. 2010, A&A, 518, L3Google Scholar
Menten, K. M. 1991, ApJ, 380, L75CrossRefGoogle Scholar
Molinari, S., Pezzuto, S., Cesaroni, R., et al. 2008, A&A, 481, 345Google Scholar
Molinari, S., Schisano, E., Faustini, F., et al. 2011, A&A, 530, A133Google Scholar
Molinari, S., Swinyard, B., Bally, J., et al. 2010, PASP, 122, 314CrossRefGoogle Scholar
Pandian, J. D. & Goldsmith, P. F. 2007, ApJ, 669, 435CrossRefGoogle Scholar
Pestalozzi, M. R., Humphreys, E. M. L., & Booth, R. S. 2002a, A&A, 384, L15Google Scholar
Pestalozzi, M. R., Minier, V., & Booth, R. S. 2005, A&A, 432, 737Google Scholar
Pestalozzi, M. R., Minier, V., Booth, R. S., & Conway, J. E. 2002b, in Cosmic Masers: from Proto-Stars to Black Holes, IAU Symposium 206, 139CrossRefGoogle Scholar
Pestalozzi, M. R., Minier, V., Motte, F., & Conway, J. E. 2006, A&A, 448, L57Google Scholar
Poglitsch, A., Waelkens, C., Geis, N., et al. 2010, A&A, 518, L2Google Scholar
Schutte, A. J., van der Walt, D. J., Gaylard, M. L., & MacLeod, G. C. 1993, MNRAS, 261, 783CrossRefGoogle Scholar
Sobolev, A. M., Cragg, D. M., & Godfrey, P. D. 1997, MNRAS, 288, L39CrossRefGoogle Scholar
Szymczak, M., Hrynek, G., & Kus, A. J. 2000, A&AS, 143, 269Google Scholar
Szymczak, M., Kus, A. J., Hrynek, G., Kepa, A., & Pazdereski, E. 2002, A&A, 392, 277Google Scholar
Traficante, A., Calzoletti, L., Veneziani, M., et al. 2011, ArXiv e-printsGoogle Scholar
van der Walt, D. J. 2005, MNRAS, 360, 153CrossRefGoogle Scholar
van der Walt, D. J., Gaylard, M. J., & MacLeod, G. C. 1995, A&AS, 110, 81Google Scholar
Walsh, A. J., Burton, M. G., Hylard, A. R., & Robinson, G. 1998, MNRAS, 301, 640CrossRefGoogle Scholar