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Galactic Fine Structure at 843 MHz

Published online by Cambridge University Press:  25 May 2016

A.J. Green ,
D. Campbell-Wilson ,
L.E. Cram ,
M.I. Large ,
B. Piestrzynski  and
T. Ye
A.J. Green
Affiliation:
University of Sydney NSW 2006, Australia
D. Campbell-Wilson
Affiliation:
University of Sydney NSW 2006, Australia
L.E. Cram
Affiliation:
University of Sydney NSW 2006, Australia
M.I. Large
Affiliation:
University of Sydney NSW 2006, Australia
B. Piestrzynski
Affiliation:
University of Sydney NSW 2006, Australia
T. Ye
Affiliation:
University of Sydney NSW 2006, Australia

Extract

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The Southern Galactic Plane surveyed by the Molonglo Observatory Synthesis Telescope (MOST) gives an unprecedented view of fine-scale structure in low frequency radio continuum emission over the area 245° ≤ l ≤ 355°, |b| ≤ 1.5°. The telescope operates at 843 MHz with a resolution of 43″ and a sensitivity of approximately 2 mJy/beam for the sample region (5° × 3°), centred on G317.5+0.0, presented here to illustrate significant features in the sources. This is a mosaic of 35 fields, each representing a 12 hr observation.

Type
Chapter 7: How are we to Understand the Small Scale Structure of the ISM?
Information
Symposium - International Astronomical Union , Volume 169: Unsolved Problems of the Milky Way , 1996 , pp. 611 - 612
Copyright
Copyright © Kluwer 1996 

References

Whiteoak, J.B.Z. (1992) Astron. Astrophys. , 262, 251 Google Scholar
Whiteoak, J.B.Z. and Green, A.J. (1994) in preparation Google Scholar