The optical supernova remnant G290.1 - 0.8
Open Access
- 1 January 1979
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 186 (1) , 45P-50P
- https://doi.org/10.1093/mnras/186.1.45p
Abstract
A photograph of the non-thermal radio source G 290.1 – 0.8 has been obtained in the light of [S II] (6717 + 6731 Å) 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 Hα/[S II] ratio.Keywords
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