XMM-Newton Discovery of 7 s Pulsations in the Isolated Neutron Star RX J1856.5-3754

Abstract

Thanks to the high counting statistics provided by a recent XMM-Newton observation of RX J1856.5-3754, we have discovered that this isolated neutron star pulsates at a period of 7.055 s. This confirms that RX J 1856.5-3754 is similar in nature to the other six thermally emitting, nearby neutron stars discovered in soft X-rays with ROSAT. The pulsations are detected at consistent periods in several XMM-Newton observations spanning from 2002 April to 2006 October, yielding an upper limit of P < 1.9 × 10 -12 s s -1 (90% c.l.) on the period derivative. This implies a surface magnetic field smaller than 1.2 × 10 14 G, under the usual assumption of vacuum dipole magnetic braking. The pulse profile is nearly sinusoidal with a pulsed fraction in the 0.15-1.2 keV range of only ∼ 1.2%, the smallest ever seen in an isolated X-ray pulsar. © 2007. The American Astronomical Society. All rights reserved.