G11.2-0.3, an evolved Cassiopeia A

Details G11.2-0.3, an evolved Cassiopeia A G11.2-0.3, an evolved Cassiopeia A

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.231..735g&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 231, April 1, 1988, p. 735-738.

Astronomy and Astrophysics

Astronomy

36

Cassiopeia A, H I Regions, Radio Astronomy, Stellar Mass, Supernova Remnants, Very Large Array (Vla), Circular Shells, Flux Density, High Resolution, Neutral Gases, Radio Sources (Astronomy)

Scientific paper

This paper presents high resolution radio observations of the relatively
bright supernova remnant G11.2-0.3 made with the VLA. These reveal a
clumpy shell of emission which resembles an evolved version of
Cassiopeia A, thus strengthening the case for association of this
remnant with the supernova of AD 386.

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