X-ray flare in 3U 0833-45 the VELA pulsar

Details X-ray flare in 3U 0833-45 the VELA pulsar X-ray flare in 3U 0833-45 the VELA pulsar

Jan 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977natur.265..121s&link_type=abstract

Nature, vol. 265, Jan. 13, 1977, p. 121-123.

Astronomy and Astrophysics

Astronomy

9

Flares, Pulsars, Supernova Remnants, X Ray Sources, Ariel 5 Satellite, Energy Dissipation, Light Curve, Magnetospheric Instability, Pulsar Magnetospheres, Sky Surveys (Astronomy)

Scientific paper

Details and implications of a flare detected from the X-ray source 3U 0833-45 (generally associated with the Vela pulsar) by the Ariel V Sky Survey Instrument are discussed. X-radiation, including synchrotron X-radiation, flare timescale data, energy stored in the magnetosphere of the Vela pulsar (PSR 0833-45), effects of release of such prodigious energy, pulsar spin effects, and shock wave phenomena are discussed. Redistribution of the magnetic field and particle flux in the pulsar magnetosphere is seen as the most probable source of the X-ray flare.

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