Hostname: page-component-78c5997874-t5tsf Total loading time: 0 Render date: 2024-11-13T12:44:28.320Z Has data issue: false hasContentIssue false

A Pilot Survey for the H2O Southern Galactic Plane Survey

Published online by Cambridge University Press:  05 March 2013

Andrew J. Walsh*
Affiliation:
Centre for Astronomy, James Cook University, Townsville, QLD 4811, Australia
Nadia Lo
Affiliation:
School of Physics, University of NSW, Sydney, NSW 2052, Australia Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 1710, Australia
Michael G. Burton
Affiliation:
School of Physics, University of NSW, Sydney, NSW 2052, Australia
Graeme L. White
Affiliation:
Centre for Astronomy, James Cook University, Townsville, QLD 4811, Australia
Cormac R. Purcell
Affiliation:
Alan Turing Building, University of Manchester, Oxford Road, Manchester, M13 9PL, UK
Steven N. Longmore
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60, Garden Street, Cambridge, MA 02138, USA
Chris J. Phillips
Affiliation:
Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 1710, Australia
Kate J. Brooks
Affiliation:
Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 1710, Australia
*
FCorresponding author. Email: andrew.walsh@jcu.edu.au
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 observations with the Mopra radiotelescope designed to assess the feasibility of the H2O Maser Southern Galactic Plane Survey. We mapped two one-square-degree regions along the Galactic plane using the new 12-mm receiver and the UNSW Mopra spectrometer. We covered the entire spectrum between 19.5 and 27.5 GHz using this setup with the main aim of finding out which spectral lines can be detected with a quick mapping survey. We report on detected emission from H2O masers, NH3 inversion transitions (1,1), (2,2) and (3,3), HC3N (3–2), as well as several radio recombination lines.

Type
Research Article
Copyright
Copyright © Astronomical Society of Australia 2008

References

Bains, I. et al., 2006, MNRAS, 367, 1609 CrossRefGoogle Scholar
Barlow, M. J. et al., 1996, A&A, 315, L241 Google Scholar
Braatz, J. A., Wilson, A. S. & Henkel, C., 1996, ApJS, 106, 51 CrossRefGoogle Scholar
Braz, M. A. & Scalise, E. Jr., 1982, A&A, 107, 272 Google Scholar
Benjamin, R. A. et al., 2003, PASP, 115, 953 CrossRefGoogle Scholar
Bergin, E. A., Maret, S., van der Tak, F. F. S., Alves, J., Carmody, S. M. & Lada, C. J., 2006, ApJ, 645, 369 CrossRefGoogle Scholar
Beuther, H., Walsh, A., Schilke, P., Sridharan, T. K., Menten, K. M. & Wyrowski, F., 2002, A&A, 390, 289 Google Scholar
Breen, S. L. et al., 2007, MNRAS, 377, 491 CrossRefGoogle Scholar
Caswell, J. L., Batchelor, R. A., Forster, J. R. & Wellington, K. J., 1989, AuJPh, 42, 331 Google Scholar
Caswell, J. L., Batchelor, R. A., Haynes, R. F. & Huchtmeier, W. K., 1974, AuJPh, 27, 417 Google Scholar
Cohen, R. J. et al., 2007, in IAU Symposium 273, Triggered Star Formation in a Turbulent ISM, Eds. Elmegreen, B. G. & Palous, J. (Cambridge: Cambridge University Press), 403 Google Scholar
Claussen, M. J. et al., 1984, ApJ, 285, L79 CrossRefGoogle Scholar
Genzel, R. & Downes, D., 1979, A&A, 72, 234 Google Scholar
Hinkle, K. H. & Barnes, T. G., 1979, ApJ, 227, 923 CrossRefGoogle Scholar
Ho, P. T. P. & Townes, C. H., 1983, ARA&A, 21, 239 Google Scholar
Johnston, K. J., Robinson, B. J., Caswell, J. L. & Batchelor, R. A., 1972, ApL, 10, 93 Google Scholar
Kaufmann, P. et al., 1976, Natur, 260, 306 CrossRefGoogle Scholar
Pandian, J. & Goldsmith, P. F., 2007, ApJ, 669, 435 CrossRefGoogle Scholar
Pillai, T., Wyrowski, F., Carey, S. J. & Menten, K. M., 2006, A&A, 450, 569 Google Scholar
Miranda, L. F., Gómez, Y., Anglada, G. & Torrelles, J. M., 2001, Natur, 414, 284 CrossRefGoogle Scholar
Mizuno, A. et al., 2001, PASJ, 53, 1071 CrossRefGoogle Scholar
Walsh, A. J. & Burton, M. G., 2006, MNRAS, 365, 321 CrossRefGoogle Scholar
Walsh, A. J., Hyland, A. R., Robinson, G. & Burton, M. G., 1997, MNRAS, 291, 261 CrossRefGoogle Scholar