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2011

The Orbit and Companion of Probable gamma-ray Pulsar J2339-0533

Romani, Roger W., Shaw, Michael S.

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We have measured dramatic flux and spectral variations through the 0.193d orbit of the optical counterpart of the unidentified gamma-ray source 0FGL J2339.8-0530.

This compact object companion is strongly heated, with T_eff varying from ~6900K (superior conjunction) to <3000K at minimum.
A combined fit to the light curve and radial velocity amplitudes implies M_1 ~ 0.075M_sun, M_2 ~ 1.4 M_sun and inclination i ~ 57deg.
Thus this is a likely `black widow' system with Edot~10^{34-34.5} erg/s pulsar driving companion mass loss.

The Orbit and Companion of Probable gamma-ray Pulsar J2339-0533 · Around

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