A new optical supernova remnant in Centaurus

Details A new optical supernova remnant in Centaurus A new optical supernova remnant in Centaurus

Sep 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974apj...192l.111i&link_type=abstract

Astrophysical Journal, vol. 192, Sept. 15, 1974, pt. 2, p. L111, L112.

Astronomy and Astrophysics

Astronomy

13

Astronomical Maps, Galactic Radiation, Light Sources, Radio Sources (Astronomy), Supernova Remnants, Centaurus Constellation, H Alpha Line, Photographic Measurement, Telescopes

Scientific paper

A filamentary nebulosity found at the position of the radio supernova remnant PKS-51/52 through photographic observations by means of the Curtis-Schmidt-type telescope at Cerro Tololo Interamerican Observatory is reported. From the observed nebulosity's filamentary structure, its blue color, and its agreement in position with the radio supernova remnant, it is concluded that it is the optical remnant of the supernova.

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