Radio Observations of the Supernova Remnant Candidate G312.5-3.0

Details Radio Observations of the Supernova Remnant Candidate G312.5-3.0 Radio Observations of the Supernova Remnant Candidate G312.5-3.0

2000-11-10

arxiv.org/abs/astro-ph/0011211v2

Mon.Not.Roy.Astron.Soc. 344 (2003) 625

Astronomy and Astrophysics

Astrophysics

5 pages, 5 figures, Accepted for publication in MNRAS

Scientific paper

10.1046/j.1365-8711.2003.06935.x

The radio images from the Parkes-MIT-NRAO (PMN) Southern Sky Survey at 4850 MHz have revealed a number of previously unknown radio sources. One such source, G312.5-3.0 (PMN J1421-6415), has been observed using the multi-frequency capabilities of the Australia Telescope Compact Array (ATCA) at frequencies of 1380 MHz and 2378 MHz. Further observations of the source were made using the Molonglo Observatory Synthesis Telescope (MOST) at a frequency of 843 MHz. The source has an angular size of 18 arcmin and has a distinct shell structure. We present the reduced multi-frequency observations of this source and provide a brief argument for its possible identification as a supernova remnant.

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