Abstract
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.
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Whiteoak J.B.Z. (1992) Astron. Astrophys., 262, 251
Whiteoak, J.B.Z. and Green, A.J. (1994) in preparation
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© 1996 Springer Science+Business Media Dordrecht
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Green, A.J., Campbell-Wilson, D., Cram, L.E., Large, M.I., Piestrzynski, B., Ye, T. (1996). Galactic Fine Structure at 843 MHZ. In: Blitz, L., Teuben, P. (eds) Unsolved Problems of the Milky Way. International Astronomical Union / Union Astronomique Internationale, vol 169. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-1687-6_98
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DOI: https://doi.org/10.1007/978-94-009-1687-6_98
Publisher Name: Springer, Dordrecht
Print ISBN: 978-0-7923-4040-9
Online ISBN: 978-94-009-1687-6
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