Implications of the millimeter emission from Supernova 1987A

Details Implications of the millimeter emission from Supernova 1987A Implications of the millimeter emission from Supernova 1987A

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...208l...5s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 208, no. 1-2, Jan. 1989, p. L5, L6.

Astronomy and Astrophysics

Astrophysics

4

Millimeter Waves, Pulsars, Supernova Remnants, Supernova 1987A, Nebulae, Periodic Variations, Synchrotron Radiation, X Ray Sources

Scientific paper

The implications of the recent detection of SN 1987A at 1.3 mm are discussed. The emission can be accounted for in terms of free-free radiation, provided that the ionized gas has a suitable filling factor. A tenable alternative is synchrotron radiation from a pulsar-powered nebula. In order to reproduce both the millimeter and the soft X-ray observations a pulsar period of 43 ms is required.

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