A Likely Redback Millisecond Pulsar Counterpart of 3FGL J0838.8-2829

Abstract

We obtained new optical observations of the X-ray source XMMU J083850.38-282756.8, the previously proposed counterpart of the gamma-ray source 3FGL J0838.8-2829. Time-series photometry in the $r^{\prime }$ band reveals periodic modulation of $\approx 1$ magnitude that is characteristic of the heating of the photosphere of a low-mass companion star by a compact object. The measured orbital period is 5.14817$\pm$0.00012 hr. The shape of the light curve is variable, evidently due to the effects of flaring and asymmetric heating. Spectroscopy reveals a companion of type M1 or later, having a radial velocity amplitude of 315$\pm$17 km/s, with period and phasing consistent with the heating interpretation. The mass function of the compact object is 0.69$\pm$0.11 $M_{\odot }$, which allows a neutron star in a high-inclination orbit. Variable, broad H$\alpha$ emission is seen, which is probably associated with a wind from the companion. These properties, as well as the X-ray and gamma-ray luminosities at the inferred distance of <1.7 kpc, are consistent with a redback millisecond pulsar in its non-accreting state. A search for radio pulsations is needed to confirm this interpretation and derive complete system parameters for modeling, although absorption by the ionized wind could hinder such detection.

arXiv comment6 pages, 4 figures, 3 tables, fixed references, published version

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