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Title: | Pulsar activity and supernova remnant morphology |
Authors: | Radhakrishnan, V. Srinivasan, G. |
Keywords: | Pulsars Stellar magnetic fields Stellar radiation Stellar structure Supernova Remnants Magnetic dipoles Magnetic flux Milky way galaxy Neutron stars Particle production Stellar evolution |
Issue Date: | 1981 |
Publisher: | Reidel |
Citation: | IAU Symposium, 1981, Vol.95, p417 |
Abstract: | The recently introduced concept of a window of magnetic field strengths in which pulsars can be active is used to explain the variation in morphology of supernova remnants. Neutron stars created with field strengths of a value permitting pulsar activity result in particle production and Crab-like, centrally-concentrated remnants. Other field values lead to strong magnetic dipole radiation and consequent shell formation, e.g., Cas A. |
Description: | Open Access. Pulsars: 13 years of research on neutron stars; Proceedings of the Symposium, Bonn, West Germany, August 26-29, 1980. (A82-32926 15-90) Dordrecht, D. Reidel Publishing Co., 1981. |
URI: | http://hdl.handle.net/2289/2452 |
Alternative Location: | http://adsabs.harvard.edu/cgi-bin/bib_query?1981IAUS...95..417R |
Copyright: | 1981 Reidel |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
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1981 IAU Symp. V95 p417.pdf Restricted Access | Open Access | 198.59 kB | Adobe PDF | View/Open Request a copy |
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