Thin Circular Disc Shells of Radio Sources Around Supernova Remnant G16.2-2.7
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Abstract
We propose a new model of distinct thin circular disc shells to analyse the radio map of the supernova remnant (SNR) G16.2-2.7 from NRAO VLA Sky Survey at 1.4 GHz and the radio sources around it. It is obtained that the 20 radio sources around the SNR G16.2-2.7 distribute on the four thin circular disc shells. The results support the shell-like structure strongly and further indicate that the shell-like structure is several thin circular disc shells. Because the shell-like structure dominate the total sample, our results is important for the research of radio mophology of SNRs.
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Cite this article:
YU Zhi-Yao. Thin Circular Disc Shells of Radio Sources Around Supernova Remnant G16.2-2.7[J]. Chin. Phys. Lett., 2002, 19(11): 1738-1740.
YU Zhi-Yao. Thin Circular Disc Shells of Radio Sources Around Supernova Remnant G16.2-2.7[J]. Chin. Phys. Lett., 2002, 19(11): 1738-1740.
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YU Zhi-Yao. Thin Circular Disc Shells of Radio Sources Around Supernova Remnant G16.2-2.7[J]. Chin. Phys. Lett., 2002, 19(11): 1738-1740.
YU Zhi-Yao. Thin Circular Disc Shells of Radio Sources Around Supernova Remnant G16.2-2.7[J]. Chin. Phys. Lett., 2002, 19(11): 1738-1740.
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