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• W2028383095 startingPage "1321" @default.
• W2028383095 abstract "Using observations made with the XMM-Newton Observatory, we report the first X-ray detection of the high magnetic field radio pulsar PSR B1916+14. We show that the X-ray spectrum of the pulsar can be well fitted with an absorbed blackbody with temperature in the range of 0.08-0.23 keV, or a neutron star hydrogen atmosphere model with best-fit effective temperature of $sim$0.10 keV, higher than expected from fast cooling models. The origin of the likely thermal emission is not well constrained by our short observation and is consistent with initial cooling or return-current heating. We found no pulsations in these data and set a 1$sigma$ upper limit on the pulsed fraction in the 0.1--2 keV band of $sim$0.7. Implications of these results for our understanding of the different observational properties of isolated neutron stars are discussed." @default.
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• W2028383095 date "2009-10-01" @default.
• W2028383095 modified "2023-10-12" @default.
• W2028383095 title "XMM-NEWTONX-RAY DETECTION OF THE HIGH-MAGNETIC-FIELD RADIO PULSAR PSR B1916+14" @default.
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• W2028383095 doi "https://doi.org/10.1088/0004-637x/704/2/1321" @default.
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