Evidence for two young galactic supernova remnants

Details Evidence for two young galactic supernova remnants Evidence for two young galactic supernova remnants

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...151l..10r&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 151, no. 2, Oct. 1985, p. L10-L12.

Astronomy and Astrophysics

Astronomy

30

Milky Way Galaxy, Radio Astronomy, Stellar Evolution, Supernova Remnants, Polarization (Waves), Radiant Flux Density, Stellar Envelopes

Scientific paper

Flux density and polarization measurements have been made of four diffuse, small diameter galactic plane sources. G54.09 + 0.26 is a polarized flat spectrum object, most likely a young plerionic-type supernova remnant (SNR). G70.68 + 1.20 is a shell-type SNR with a size of less than 1.5 pc. It is most likely the youngest galactic SNR known so far. The nature of G50.29-0.40 and G71.23 + 1.47 remains unclear.

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