K. O. Mason, J. L. Culhane
Abstract
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Investigation of the X-ray source associated with PSR 0833 – 45, using data from the Copernicus and Ariel V satellites, indicates a significant enhancement in surface brightness within 6 arcmin of the pulsar, while confirming that the emission is extended.
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Investigation of the X-ray source associated with PSR 0833 – 45, using data from the Copernicus and Ariel V satellites, indicates a significant enhancement in surface brightness within 6 arcmin of the pulsar, while confirming that the emission is extended.
Key concepts: Physics, Vela, Pulsar, Astrophysics, Copernicus, Astronomy, Surface brightness, Brightness