G357.7 + 0.3 and G359.1 - 0.5 - Two shell-type supernova remnants in the galactic centre region

Details G357.7 + 0.3 and G359.1 - 0.5 - Two shell-type supernova remnants in the galactic centre region G357.7 + 0.3 and G359.1 - 0.5 - Two shell-type supernova remnants in the galactic centre region

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26as...57..165r&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 57, July 1984, p. 165-167.

Astronomy and Astrophysics

Astrophysics

31

Galactic Nuclei, Milky Way Galaxy, Radio Spectra, Stellar Envelopes, Supernova Remnants, Astronomical Maps, Centimeter Waves, Continuous Spectra, Linear Polarization, Spectral Energy Distribution

Scientific paper

A new shell-type supernova remnant (SNR), G357.7+0.3, has been
identified from radio continuum observations at 11 cm and 6 cm
wavelength. G359.1-0.5 was previously suggested to be a SNR by Downes et
al. (1978) from its morphology. A study of spectral index and linear
polarization confirm the object to be a SNR.

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