Abstract
The XMM-Newton spectra of the isolated neutron star RXJ0720.4-3125 obtained over 4.5 years can be described by sinusoidal variations in the inferred blackbody temperature, the size of the emitting a e and the depth of the absorption line with a period of 7.1 +/- 0.5 years, which we suggest to be the precession period of the neutron star. Precession of a neutron star with two hot spots of different temperature and size, probably not located exactly in anti positions, may account for the variations in the X-ray spectra, changes in the pulsed fraction, shape of the light curve and the phase-lag between soft and hard energy bands observed from RXJ0720.4-3125. An independent sinusoidal fit to published and new pulse timing residuals from a coherent analysis covering similar to 12 years yields a consistent period of 7.7 +/- 0.6 years supporting the precession model.
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