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arXiv · 1511.04233

Near-infrared observations of PSR J1357-6429

D. Zyuzin·S. Zharikov·Yu. Shibanov·A. Danilenko·R. E. Mennickent·A. Kirichenko
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Abstract

PSR J1357$-$6429 is a young radio pulsar that was detected in X-rays and $γ$-rays. We present the high spatial resolution near-infrared imaging of the pulsar field in $J$, $H$ and $K_s$ bands obtained with the VLT/NaCo using the Adaptive Optic system. We found a faint source at the most precise pulsar radio position which we propose as the pulsar near-infrared counterpart candidate. It is confidently detected in the $J$ and $K_s$ bands, with $J$ = 23.51$\pm$0.24 and $K_s$ = 21.82$\pm$0.25. There is a hint of the source in the $H$ band with an upper limit $H$ $>$ 22.8. The dereddened source fluxes are compatible with the extrapolation of the pulsar X-ray spectrum towards the near-infrared. If the candidate is the true counterpart, by this property PSR J1357$-$6429 would be similar to the nearby middle-age pulsar PSR B0656+14. In this case, both pulsars demonstrate an unusually high near-infrared efficiency relative to the X-ray efficiency as compared to other pulsars detected in both ranges.

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D. Zyuzin, S. Zharikov, Yu. Shibanov, A. Danilenko, R. E. Mennickent, A. Kirichenko. 2016-02-17. Near-infrared observations of PSR J1357-6429. https://doi.org/10.1093/mnras%2Fstv2401

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