XMM-NEWTONX-RAY OBSERVATION OF THE HIGH-MAGNETIC-FIELD RADIO PULSAR PSR J1734–3333
نویسندگان
چکیده
منابع مشابه
Radio Polarization of the Young High - Magnetic - Field Pulsar Psr
We have investigated the radio polarization properties of PSR J1119−6127, a recently discovered young radio pulsar with a large magnetic field. Using pulsar-gated radio imaging data taken at a center frequency of 2496 MHz with the Australia Telescope Compact Array, we have determined a rotation measure for the pulsar of +842± 23 rad m. These data, combined with archival polarimetry data taken a...
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PSR J1814−1744 is a 4 s radio pulsar with surface dipole magnetic field strength 5.5× 10 G, inferred assuming simple magnetic dipole braking. This pulsar’s spin parameters are very similar to those of anomalous X-ray pulsars (AXPs), suggesting that this may be a transition object between the radio pulsar and AXP population, if AXPs are isolated, high magnetic field neutron stars as has recently...
متن کاملRadio Polarization of the Young High-Magnetic-Field Pulsar PSR J1119-6127
We have investigated the radio polarization properties of PSR J1119 6127, a recently discovered young radio pulsar with a large magnetic field. Using pulsar-gated radio imaging data taken at a center frequency of 2496 MHz with the Australia Telescope Compact Array, we have determined a rotation measure for the pulsar of +842 23 rad m 2. These data, combined with archival polarimetry data taken ...
متن کاملDetection of the High Magnetic Field Radio Pulsar PSR B 1916 + 14
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 ∼0.10 keV, higher than expe...
متن کاملUnusual Pulsed X - Ray Emission from the Young , High Magnetic Field Pulsar Psr J 1119 – 6127
We present XMM–Newton observations of the radio pulsar PSR J1119–6127, which has an inferred age of 1,700 yr and surface dipole magnetic field strength of 4.1×10 13 G. We report the first detection of pulsed X-ray emission from PSR J1119–6127. In the 0.5–2.0 keV range, the pulse profile shows a narrow peak with a very high pulsed fraction of (74±14)%. In the 2.0–10.0 keV range, the upper limit ...
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ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 2010
ISSN: 0004-637X,1538-4357
DOI: 10.1088/0004-637x/725/1/985