Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...126....7b&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 126, no. 1, Sept. 1983, p. 7-9. Research supported by the Ministero della Pubb
Astronomy and Astrophysics
Astrophysics
26
Crab Nebula, Pulsars, Supernovae, Explosions, Filaments, Stellar Envelopes, Supernova Remnants, Taylor Instability
Scientific paper
It is determined that filaments from supernova remnants are formed before a substantial interaction with the interstellar medium has taken place. It is argued that the envelope in supernovae with a central pulsar is fragmented shortly after the explosion because of a Rayleigh-Taylor instability. The emission from a pulsar-powered bubble is determined to then become visible, in agreement with the radio supernovae phenomenon. These findings are shown to agree with the commonly accepted evolutionary scheme of the Crab Nebula, and account for the detection of radio emission from recent Type II supernovae.
Bandiera Rino
Pacini Franco
Salvati Marco
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