Hostname: page-component-8448b6f56d-wq2xx Total loading time: 0 Render date: 2024-04-24T23:07:47.917Z Has data issue: false hasContentIssue false
  • English
  • Français

The RMS survey: Massive young stars throughout the galaxy

Published online by Cambridge University Press:  08 November 2005

M. G. Hoare ,
S. L. Lumsden ,
R. D. Oudmaijer ,
J. S. Urquhart ,
A. L. Busfield ,
T. L. Sheret ,
A. J. Clarke ,
T. J. T. Moore ,
J. Allsopp  and
M. G. Burton
...Show all authors
M. G. Hoare
Affiliation:
School of Physics and Astronomy, University of Leeds, LS2 9JT, UK email: mgh@ast.leeds.ac.uk
S. L. Lumsden
Affiliation:
School of Physics and Astronomy, University of Leeds, LS2 9JT, UK email: mgh@ast.leeds.ac.uk
R. D. Oudmaijer
Affiliation:
School of Physics and Astronomy, University of Leeds, LS2 9JT, UK email: mgh@ast.leeds.ac.uk
J. S. Urquhart
Affiliation:
School of Physics and Astronomy, University of Leeds, LS2 9JT, UK email: mgh@ast.leeds.ac.uk
A. L. Busfield
Affiliation:
School of Physics and Astronomy, University of Leeds, LS2 9JT, UK email: mgh@ast.leeds.ac.uk
T. L. Sheret
Affiliation:
School of Physics and Astronomy, University of Leeds, LS2 9JT, UK email: mgh@ast.leeds.ac.uk
A. J. Clarke
Affiliation:
School of Physics and Astronomy, University of Leeds, LS2 9JT, UK email: mgh@ast.leeds.ac.uk
T. J. T. Moore
Affiliation:
Institute for Astrophysical Research, Liverpool John Moores University Twelve Quays House, Egerton Wharf, Birkenhead, UK
J. Allsopp
Affiliation:
Institute for Astrophysical Research, Liverpool John Moores University Twelve Quays House, Egerton Wharf, Birkenhead, UK
M. G. Burton
Affiliation:
School of Physics, University of New South Wales, Sydney, Australia
C. R. Purcell
Affiliation:
School of Physics, University of New South Wales, Sydney, Australia
Z. Jiang
Affiliation:
Purple Mountain Observatory, Nanjing, P. R. China
M. Wang
Affiliation:
Purple Mountain Observatory, Nanjing, P. R. China
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.

We describe a programme that aims to increase the known sample of massive young stellar objects (MYSOs) by an order of magnitude. About 2000 candidates colour-selected from the MSX survey are being followed up at radio, mm and IR wavelengths to identify genuine MYSOs from the UCHII regions and other contaminants. Results so far indicate that the strategy does indeed deliver a significant fraction of luminous YSOs that will provide the basis for future galaxy-wide systematic studies.

Keywords

infrared: starsradio continuum: ISMradio lines: ISMstars: formationH II regions
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 1 , Symposium S227: Massive Star Birth: A Crossroads of Astrophysics , May 2005 , pp. 370 - 375
Copyright
© 2005 International Astronomical Union