Two new filled-center supernova remnants - G24.7+0.6 and G27.8+0.6

Details Two new filled-center supernova remnants - G24.7+0.6 and G27.8+0.6 Two new filled-center supernova remnants - G24.7+0.6 and G27.8+0.6

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...133l...4r&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 133, no. 1, April 1984, p. L4-L7.

Astronomy and Astrophysics

Astronomy

37

Astronomical Maps, Radio Sources (Astronomy), Stellar Evolution, Supernova Remnants, Centimeter Waves, Crab Nebula, Linear Polarization, Radiant Flux Density, Radio Spectra

Scientific paper

As is true for most filled centers, the two objects have no clear boundaries; this makes estimates of the dimensions, distances, and ages somewhat ambiguous. Even though the derived quantities are still not accurate, it is believed that the two objects may provide promising clues in investigations of the late stage of evolution of Crab-like SNRs. In both objects, the centrally peaked sources are seen as suggesting some energetic sources at the centers. It is pointed out that the central region of G24.7+0.6 is not resolved in the observations and appears to be associated with a plateaulike or jetlike extension toward the west. The objects are linearly polarized, indicating their nonthermal origin.

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