A study of the composite supernova remnant G 18.95-1.1

Details A study of the composite supernova remnant G 18.95-1.1 A study of the composite supernova remnant G 18.95-1.1

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...209..361f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 209, no. 1-2, Jan. 1989, p. 361-368.

Astronomy and Astrophysics

Astrophysics

13

Astronomical Spectroscopy, Pulsars, Radio Emission, Supernova Remnants, Brightness Distribution, Continuous Radiation, H Lines, Stellar Luminosity, Very Large Array (Vla)

Scientific paper

Radio continuum and H I 21-cm line observations of the galactic nonthermal object, G 18.95-1.1, are discussed. The object has a spectral index of -0.28 between 57.5 MHz and 10 GHz. Based on its morphology and spectral characteristics, G 18.95-1.1 is classified as a composite supernova remnant. H I line data show a depression in antenna temperature of the extent of the object at 18 km/s giving a distance of 2 kpc.

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