What is the nature of RX J0720.4-3125?
arXiv:astro-ph/9801038 · doi:10.1046/j.1365-8711.1998.01799.x
Abstract
RX J0720.4-3125 has recently been identified as a pulsating soft X-ray source in the ROSAT all-sky survey with a period of 8.391 s. Its spectrum is well characterized by a black-body with a temperature of K. We propose that the radiation from this object is thermal emission from a cooling neutron star. For this black-body temperature we can obtain a robust estimate of the object's age of yr, yielding a polar field G for magnetic-dipole spin down and a value of compatible with current observations.
4 pages, 1 figures, to appear in Monthly Notices
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