A Coherent Timing Solution for the Nearby, Thermally Emitting Isolated Neutron Star RX J0420.0-5022
David L. Kaplan, Marten H. van Kerkwijk

TL;DR
This paper provides a precise phase-coherent timing solution for the neutron star RX J0420.0-5022, revealing its magnetic field and age, and compares it with other isolated neutron stars to understand their evolution.
Contribution
It offers the first coherent timing solution for RX J0420.0-5022, extending previous observations and refining measurements of its magnetic field and spin-down rate.
Findings
RX J0420.0-5022 has the lowest dipole magnetic field among INSs.
All 6 INSs with confirmed periodicities now have constrained spin-downs.
INSs are likely older and hotter than rotation-powered pulsars of similar age.
Abstract
We present a phase-coherent timing solution for RX J0420.0-5022, the coolest (kT=45 eV) and fastest-spinning (P=3.45 s) of the seven so-called isolated neutron stars (INSs). Using 14 observations with the XMM-Newton spacecraft in 2010-2011, we were able to measure a spin-down rate nudot=(-2.3+/-0.2)e-15 Hz/s (Pdot=(2.8+/-0.3)e-14 s/s), from which we infer a dipolar magnetic field of 1.0e13 G. With reasonable confidence we were able to extend the timing solution back to archival XMM-Newton from 2002 and 2003, giving the same solution but with considerably more precision. This gives RX J0420 the lowest dipole magnetic field of the INSs. Our spectroscopy does not confirm the broad absorption feature at 0.3 keV hinted at in earlier observations, although difficulties in background subtraction near that energy make conclusions difficult. With this, all 6 of the INSs that have confirmed…
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