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Blind HI Survey in the Great Attractor Region

Published online by Cambridge University Press:  05 March 2013

S. Juraszek
S. Juraszek*
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia; [email protected] Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 2121, Australia; [email protected]
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Abstract

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Optically, the Zone of Avoidance (ZOA) can only be explored to within a few degrees of the Galactic Equator. This restriction does not apply to radio wavelengths where we are able to detect galaxies at great distances behind the Galactic Plane. Using the Parkes 21 cm multibeam instrument we have detected neutral hydrogen (HI) in 42 galaxies in the region of the Great Attractor. We have been able to identify nine galaxies and make positional associations with a further six from existing optical catalogues, which makes at least 60% of these galaxies new discoveries.

Keywords

surveysgalaxies: distances and redshiftsgalaxies: fundamental parametersradio lines: galaxies
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 16 , Issue 1 , 1999 , pp. 38 - 41
Copyright
Copyright © Astronomical Society of Australia 1999

References

Barnes, D. G. 1998, in ADASS VII (San Francisco: ASP), p. 32 Google Scholar
Cao, Y., Terebey, S., Prince, T. A., & Beichman, C. A. 1997, ApJ, Suppl., 111, 387 Google Scholar
Durand, N., Bottinelli, L., Gouguenheim, L., Paturel, G., Gamier, R., Marthinet, M. C., & Petit, C. 1994, in Unveiling Large-scale Structures behind the Milky Way, ASP Conf Ser. 67, eds C. Balkowski & R. C. Kraan-Korteweg (San Francisco: ASP), p. 257 Google Scholar
Frater, R. H., & Brooks, J. W. 1992, J. Electr. Electron. Eng. Aust. (special issue), 12, no. 2, JuneGoogle Scholar
IRAS Point Source Catalogue 1998, Version 2, Joint IRAS Science Working Group (Washington: GPO)Google Scholar
Kraan-Korteweg, R. C. 1996, Nature, 379, 519 Google Scholar
Kraan-Korteweg, R. C., Loan, A. J., Burton, W. B., Lahav, O., Ferguson, H. C., Henning, P. A., & Lynden-Bell, D. 1994, Nature, 372, 77 Google Scholar
Kraan-Korteweg, R. C., Woudt, P. A., & Henning, P. A. 1997, PASA, 14, 15 Google Scholar
Lu, N. Y., Dow, M. W., Houck, J. R., Salpeter, E. E., & Lewis, B. M. 1990, ApJ, 357, 388 CrossRefGoogle Scholar
Staveley-Smith, L. 1997, PASA, 14, 111 CrossRefGoogle Scholar
Staveley-Smith, L., Juraszek, S., Koribalski, B. S., Ekers, R. D., Green, A. J., Haynes, R. F., Henning, P. A., Kesteven, M. J., Kraan-Korteweg, R. C., Price, R. M., & Sadler, E. M. 1998, AJ, 116, 2717 Google Scholar