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arXiv · 2105.07779

IKT16: Discovery of a 22 ms energetic rotation-powered pulsar in the Small Magellanic Cloud

C. Maitra·P. Esposito·A. Tiengo·J. Ballet·F. Haberl·S. Dai·M. D. Filipovic·M. Pilia
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Abstract

We report here on the discovery with XMM-Newton of pulsations at 22 ms from the central compact source associated with IKT16, a supernova remnant in the Small Magellanic Cloud (SMC). The measured spin period and spin period derivative correspond to 21.7661076(2) ms and $2.9(3)\times10^{-14}$ s,s$^{-1}$, respectively. Assuming standard spin-down by magnetic dipole radiation, the spin-down power corresponds to $1.1\times10^{38}$,erg,s$^{-1}$ implying a Crab-like pulsar. This makes it the most energetic pulsar discovered in the SMC so far and a close analogue of PSR J0537--6910, a Crab-like pulsar in the Large Magellanic Cloud. The characteristic age of the pulsar is 12 kyr. Having for the first time a period measure for this source, we also searched for the signal in archival data collected in radio with the Parkes telescope and in Gamma-rays with the Fermi/LAT, but no evidence for pulsation was found in these energy bands.

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C. Maitra, P. Esposito, A. Tiengo, J. Ballet, F. Haberl, S. Dai, M. D. Filipovic, M. Pilia. 2021-05-17. IKT16: Discovery of a 22 ms energetic rotation-powered pulsar in the Small Magellanic Cloud. https://doi.org/10.1093/mnrasl%2Fslab050

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