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arXiv · 0707.3037

The optical counterpart of IGR J00291+5934 in quiescence

P. D'Avanzo·S. Campana·S. Covino·G. L. Israel·L. Stella·G. Andreuzzi
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Abstract

The recent (December 2004) discovery of the sixth accretion-powered millisecond X-ray pulsar IGR J00291+5934 provides a very good chance to deepen our knowledge of such systems. Although these systems are well studied at high energies, poor informations are available for their optical/NIR counterparts during quiescence. Up to now, only for SAX J1808.4-3658, the first discovered system of this type, we have a secure multiband detection of its optical counterpart in quiescence. Among the seven known system IGR J00291+5934 is the one that resembles SAX J1808.4-3658 more closely. With the Italian 3.6 m TNG telescope, we have performed deep optical and NIR photometry of the field of IGR J00291+5934 during quiescence in order to look for the presence of a variable counterpart. We present here the first multiband ($VRIJH$) detection of the optical and NIR counterpart of IGR J00291+5934 in quiescence as well as a deep upper limit in the $K-$band. We obtain an optical light curve that shows variability consistent with a sinusoidal modulation at the known 2.46 hr orbital period and present evidence for a strongly irradiated companion.

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P. D'Avanzo, S. Campana, S. Covino, G. L. Israel, L. Stella, G. Andreuzzi. 2007-07-20. The optical counterpart of IGR J00291+5934 in quiescence. https://doi.org/10.1051/0004-6361%3A20077395

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