The optical supernova remnant G290.1-0.8

Details The optical supernova remnant G290.1-0.8 The optical supernova remnant G290.1-0.8

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.186p..45e&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 186, Mar. 1979, p. 45P-50P.

Astronomy and Astrophysics

Astronomy

12

Astronomical Photography, Optical Emission Spectroscopy, Radio Sources (Astronomy), Stellar Spectra, Supernova Remnants, Visual Observation, Filaments, H Alpha Line, Hydrogen Clouds, Nonthermal Radiation

Scientific paper

A photograph of the nonthermal radio source G290.1-0.8 has been obtained in the light of forbidden S II (6717+6731 A) at the prime focus of the Anglo-Australian Telescope. The plate shows a circular patch of emission and a number of filaments coincident with the steep edge of the radio shell. The filaments have spectra typical of supernova remnants with low values of the H-alpha/forbidden S II ratio.

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