S Roy and S Bhatnagar 2006 J. Phys.: Conf. Ser. 54 152 doi:10.1088/1742-6596/54/1/025
S Roy1 and S Bhatnagar2
Show affiliationsWe have made deep observations with the GMRT at 330 MHz of seven, yet- unclassified objects in the Molonglo Galactic Centre Survey (MGCS) in order to confirm the nature of these sources. Based on morphology and non-thermal spectral indices, five of them are now confirmed to be SNRs. This makes the number density of SNRs in the region a factor of two higher than expected from a smooth distribution of SNRs in the Galaxy.
95.55.Jz Radio telescopes and instrumentation; heterodyne receivers
Issue 1 (2006)
S Roy and S Bhatnagar 2006 J. Phys.: Conf. Ser. 54 152
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F Pavese and G T McConville 1987 Metrologia 24 107
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Jeffrey D Martin and Steven D Hudson 2009 New J. Phys. 11 115005
Cao Bing-Yang et al 2004 Chinese Phys. Lett. 21 1777
Alexander Moroz 1996 J. Phys. A: Math. Gen. 29 289
Dexin Zhong and D Ben-Avraham 1995 J. Phys. A: Math. Gen. 28 33
Mingtao Li et al 2003 Nanotechnology 14 33
E Caliceti and S Graffi 2004 J. Phys. A: Math. Gen. 37 2239