When Will a Pulsar in Supernova 1987a Be Seen?
Author:
Affiliation:
1. Kellogg Radiation Laboratory, California Institute of Technology, Pasadena, CA 91125.
2. Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA 91125.
Publisher
American Association for the Advancement of Science (AAAS)
Subject
Multidisciplinary
Reference30 articles.
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2. BAHCALL, J, EXTRAGALACTIC PULSARS, ASTROPHYSICAL JOURNAL 162: 737 (1970).
3. BARBON, R, PHOTOMETRIC PROPERTIES OF TYPE-II SUPER-NOVAE, ASTRONOMY AND ASTROPHYSICS 72: 287 (1979).
4. BIONTA, R.M., OBSERVATION OF A NEUTRINO BURST IN COINCIDENCE WITH SUPERNOVA 1987A IN THE LARGE MAGELLANIC CLOUD, PHYSICAL REVIEW LETTERS 58: 1494 (1987).
5. BLANDFORD, R.D., THERMAL ORIGIN OF NEUTRON STAR MAGNETIC-FIELDS, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 204: 1025 (1983).
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1. Neutron star magnetic field dynamics and its evolution;Monthly Notices of the Royal Astronomical Society;1996-10
2. A Search for a Pulsar in the Remnant of SN 1987A with the Hubble Space Telescope High-Speed Photometer;The Astrophysical Journal;1995-06
3. Passive and active seti strategies using the synchronization of SN1987A;Astrophysics and Space Science;1994-04
4. Cosmic ray acceleration in pulsar-driven supernova remnants;Monthly Notices of the Royal Astronomical Society;1992-08-01
5. Confirmation of dust condensation in the ejecta of supernova 1987a.;Proceedings of the National Academy of Sciences;1990-06-01
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