Supernova remnants and their neutron stars

Details Supernova remnants and their neutron stars Supernova remnants and their neutron stars

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001a%26at...20..207d&link_type=abstract

Astronomical and Astrophysical Transactions, vol. 20, Issue 2, pp.207-214

Astronomy and Astrophysics

Astronomy

Ism, Snrs, Pulsars, Neutron Stars

Scientific paper

Both plerionic and composite supernova remnants with interior pulsars show a great variety of interactions between the pulsar and the surrounding remnant. Those objects without detected pulsars show the same kinds of characteristics and are otherwise indistinguishable from those in which the pulsar is seen. Other shell SNRs show interior cooling neutron stars or pulsars but no apparent connection between the shells and the neutron stars. A large range of progenitor characteristics and circumstellar environments must be needed to produce the differences among these supernova remnants.

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