Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...340..355b&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 340, May 1, 1989, p. 355-361.
Astronomy and Astrophysics
Astrophysics
77
Nebulae, Pulsars, Stellar Evolution, Supernova Remnants, Astronomical Maps, Crab Nebula, Luminosity, Very Large Array (Vla)
Scientific paper
Data for fields containing three of the youngest known pulsars reveal little radiation which can be attributable to supernova remnants associated with their formation. The present observations suggest a mean observable lifetime of less than about 20,000 yr for both pulsar and blast-wave powered remnants. The relatively rapid luminosity decline of both of these phenomena can be explained by a scenario in which the most massive supernova occurs within regions of low density bounded at radii of 10-30 pc by high-density shells.
Braun Robert
Goss William Miller
Lyne Andrew G.
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