The galactic radio sources G5.4 - 1.2 and G5.27 - 0.90

Details The galactic radio sources G5.4 - 1.2 and G5.27 - 0.90 The galactic radio sources G5.4 - 1.2 and G5.27 - 0.90

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.225..329c&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 225, March 15, 1987, p. 329-334.

Astronomy and Astrophysics

Astronomy

31

Milky Way Galaxy, Radio Sources (Astronomy), Supernova Remnants, Astronomical Maps, Brightness Distribution, Nebulae, Nonthermal Radiation, Pulsars

Scientific paper

A new map at 843 MHz indicates that G5.4 - 1.2 is a supernova remnant of the shell variety with diameter 35 arcmin. Nearby lies G5.27 - 0.90, a nonthermal radio source (diameter only about 1 arcmin) with similarities to the Crab Nebula, and perhaps excited by a recently detected short-period radio pulsar. A 'tail' extends from the nebula G5.27 - 0.90 towards the shell of G5.4 - 1.2, raising the possibility that G5.27 0.90 was ejected from the shell remnant.

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