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New Galactic ISM results and progress towards low-frequency spectroscopy

Published online by Cambridge University Press:  01 August 2006

Anne J. Green ,
Tara Murphy ,
Duncan Campbell-Wilson ,
Michael Kesteven  and
John Bunton
Anne J. Green
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia email: agreen@physics.usyd.edu.au
Tara Murphy
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia email: agreen@physics.usyd.edu.au
Duncan Campbell-Wilson
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia email: agreen@physics.usyd.edu.au
Michael Kesteven
Affiliation:
CSIRO Australia Telescope National Facility, PO Box 76, Epping, NSW 1710, Australia
John Bunton
Affiliation:
CSIRO Australia Telescope National Facility, PO Box 76, Epping, NSW 1710, Australia
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Abstract

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We dicuss new Galactic ISM results and progress towards low-frequency spectroscopy

Keywords

radio continuum: ISMstars: formationISM: supernova remnantssurveys

References

Bock, D.-C. J, Large, M. I., & Sadler, E. M. 1999, AJ, 117, 1578CrossRefGoogle Scholar
Cohen, M., & Green, A. J. 2001, MNRAS, 325, 531CrossRefGoogle Scholar
Green, A. J. 2002 in: Rao, A. P., Swarup, G. & Gopal-Krishna, (eds.), The Universe at Low Radio Frequencies, Proc. IAU Symposium No. 199 (San Francisco: ASP), p. 259CrossRefGoogle Scholar