Data

Parkes observations for project P834 semester 2013OCTS

The University of Western Australia
Staveley-Smith, Lister ; Manchester, Dick ; Zanardo, Giovanna
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ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Adc&rfr_id=info%3Asid%2FANDS&rft_id=info:doi10.4225/08/560bf966bdca1&rft.title=Parkes observations for project P834 semester 2013OCTS&rft.identifier=10.4225/08/560bf966bdca1&rft.publisher=CSIRO Publishing&rft.description=We propose to search for a pulsar in the remnant of SN1987A. The existence of a neutron star formed after the explosion of the progenitor, Sk ?69?202, is predicted by stellar evolution theory. Early neutrino detection by three separate ground-based detectors appears to confirm the formation of neutrons. Moreover, recent Compact Array observations hint at the presence of a flat-spectrum component near the centre of the remnant, possibly the result of synchrotron emission from a pulsar-powered nebula. However, the initial mass of the SN1987A progenitor is close to the limit where collapse into a black hole is predicted. It is therefore possible that fallback of matter onto the neutron star resulted in later formation of a black hole, or even a quark star. Detection or otherwise of the SN1987A pulsar would make a powerful contribution to stellar evolution theory.&rft.creator=Staveley-Smith, Lister &rft.creator=Manchester, Dick &rft.creator=Zanardo, Giovanna &rft.date=2014&rft.type=dataset&rft.language=English Access the data

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We propose to search for a pulsar in the remnant of SN1987A. The existence of a neutron star formed after the explosion of the progenitor, Sk ?69?202, is predicted by stellar evolution theory. Early neutrino detection by three separate ground-based detectors appears to confirm the formation of neutrons. Moreover, recent Compact Array observations hint at the presence of a flat-spectrum component near the centre of the remnant, possibly the result of synchrotron emission from a pulsar-powered nebula. However, the initial mass of the SN1987A progenitor is close to the limit where collapse into a black hole is predicted. It is therefore possible that fallback of matter onto the neutron star resulted in later formation of a black hole, or even a quark star. Detection or otherwise of the SN1987A pulsar would make a powerful contribution to stellar evolution theory.

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Associated Persons
Giovanna Zanardo (Creator)Dick Manchester (Creator)

Issued: 2014-01-01

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