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- W2162280495 abstract "We observed the 3.8 s pulsar CXOU J171405.7|$-$|381031 with XMM-Newton, and discovered a significant |$dot P$| of 6.40|$ pm $|0.05 |$times$| 10|$^{-11} $|s s|$^{-1}$| from this source for the first time, with the aid of archival Chandra data. The characteristic age (950 yr), the magnetic field strength (5 |$times$| 10|$^{14} $|G), and the spin-down luminosity (4.5 |$times$| 10|$^{34} $|erg s|$^{-1}$|) derived from |$P$| and |$dot P$| lead us to conclude that CXOU J171405.7|$-$|381031 should be identified as a new magnetar. The obtained characteristic age indicates that CXOU J171405.7|$-$|381031 is the youngest among all known anomalous X-ray pulsars, and is consistent with the age estimated from the thermal X-rays of the associated supernova remnant. The ratio between the 2–10 keV luminosity and the spin-down luminosity is almost unity, which implies that CXOU J171405.7|$-$|381031 is the key source to connect magnetars with traditional radio pulsars." @default.
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- W2162280495 date "2010-10-25" @default.
- W2162280495 modified "2023-09-27" @default.
- W2162280495 title "Identification of CXOU J171405.7−381031 as a New Magnetar with XMM-Newton" @default.
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- W2162280495 doi "https://doi.org/10.1093/pasj/62.5.l33" @default.
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