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相关论文: Discovery of X-ray Pulsations from the INTEGRAL So…

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We report the discovery of 31.18 ms pulsations from the INTEGRAL source IGR J14003-6326 using the Rossi X-ray Timing Explorer (RXTE). This pulsar is most likely associated with the bright Chandra X-ray point source lying at the center of…

高能天体物理现象 · 物理学 2014-11-20 M. Renaud , V. Marandon , E. V. Gotthelf , J. Rodriguez , R. Terrier , F. Mattana , F. Lebrun , J. A. Tomsick , R. N. Manchester

We report on Chandra X-ray and Parkes radio observations of IGR J11014-6103, which is a possible pulsar wind nebula with a complex X-ray morphology and a likely radio counterpart. With the superb angular resolution of Chandra, we find…

We report the discovery and follow-up timing observations of the 63 ms radio pulsar, PSR J1105-6107. The pulsar is young, having a characteristic age of only 63 kyr and, from its dispersion measure, is estimated to be at a distance of ~7…

天体物理学 · 物理学 2009-10-30 V. M. Kaspi , M. Bailes , R. N. Manchester , B. W. Stappers , J. S. Sandhu , J. Navarro , N. D'Amico

PSR J1101-6101 is an energetic young pulsar which powers the remarkable Lighthouse pulsar wind nebula (PWN). The pulsar belongs to the rare type of radio- and gamma-ray-quiet pulsars which are bright in hard X-rays. Moreover, the Lighthouse…

高能天体物理现象 · 物理学 2023-07-05 Noel Klingler , Jeremy Hare , Oleg Kargaltsev , George G. Pavlov , John Tomsick

Context: IGRJ11014-6103 is one of the still unidentified hard X-ray INTEGRAL sources, reported for the first time in the 4th IBIS/ISGRI catalog. Aims: We investigated the nature of IGR J11014-6103 by carrying out a multiwavelength analysis…

高能天体物理现象 · 物理学 2013-03-20 L. Pavan , E. Bozzo , G. Pühlhofer , C. Ferrigno , M. Balbo , R. Walter

With a period of 51.6 ms and spin-down power 2.2x10^{37} erg s^{-1}, PSR J2229+6114 is a compelling identification for the EGRET source 3EG J2227+6122 in which error circle it resides. Striking features of the Chandra X-ray image are an…

天体物理学 · 物理学 2007-05-23 J. P. Halpern , E. V. Gotthelf , F. Camilo , B. Collins , D. J. Helfand

We have investigated the field around the radio-quiet $\gamma$-ray pulsar, PSR J2021+4026, with a ~140 ks XMM-Newton observation and a ~56 ks archival Chandra data. Through analyzing the pulsed spectrum, we show that the X-ray pulsation is…

高能天体物理现象 · 物理学 2015-06-23 C. Y. Hui , K. A. Seo , L. C. C. Lin , R. H. H. Huang , C. P. Hu , J. H. K. Wu , L. Trepl , J. Takata , Y. Wang , Y. Chou , K. S. Cheng , A. K. H. Kong

We report the discovery of a 38.5 ms X-ray pulsar in observations of the soft gamma-ray source IGR J18490-0000 with the Rossi X-ray Timing Explorer (RXTE). PSR J1849-0001 is spinning down rapidly with period derivative 1.42E-14 s/s,…

高能天体物理现象 · 物理学 2015-05-20 E. V. Gotthelf , J. P. Halpern , R. Terrier , F. Mattana

We present Chandra X-ray Observatory imaging observations of the young Galactic supernova remnant G11.2-0.3. The image shows that the previously known young 65-ms X-ray pulsar is at position (J2000) RA 18h 11m 29.22s, DEC -19o 25' 27.''6,…

天体物理学 · 物理学 2009-11-06 V. M. Kaspi , M. E. Roberts , G. Vasisht , E. V. Gotthelf , M. Pivovaroff , N. Kawai

We report the discovery with the Parkes radio telescope of a pulsar associated with the ~ 1700 yr-old oxygen-rich composite supernova remnant G292.0+1.8. PSR J1124-5916 has period 135 ms and period derivative 7.4e-13, implying…

天体物理学 · 物理学 2009-11-07 F. Camilo , R. N. Manchester , B. M. Gaensler , D. R. Lorimer , J. Sarkissian

We report the discovery of 44.7 ms pulsations from the X-ray source CXOU J181335.1-174957 using data obtained with the XMM-Newton Observatory. PSR J1813-1749 lies near the center of the young radio supernova remnant G12.82-0.02, which…

高能天体物理现象 · 物理学 2009-07-22 E. V. Gotthelf , J. P. Halpern

Jets from rotation-powered pulsars have so far only been observed in systems moving subsonically trough their ambient medium and/or embedded in their progenitor supernova remnant (SNR). Supersonic runaway pulsars are also expected to…

高能天体物理现象 · 物理学 2015-06-17 L. Pavan , P. Bordas , G. Puehlhofer , M. D. Filipovic , A. De Horta , A. O'Brien , M. Balbo , R. Walter , E. Bozzo , C. Ferrigno , E. Crawford , L. Stella

We report the discovery of a 206 ms pulsar associated with the TeV gamma-ray source HESS J1640-465 using the Nuclear Spectroscopic Telescope Array (NuSTAR) X-ray observatory. PSR J1640-4631 lies within the shell-type supernova remnant (SNR)…

We report the discovery of a pulsar with period P = 136 ms and dispersion measure 308 pc/cc in a deep observation of the supernova remnant (SNR) G54.1+0.3 with the Arecibo radio telescope. Timing measurements of the new pulsar, J1930+1852,…

天体物理学 · 物理学 2009-11-07 F. Camilo , D. R. Lorimer , N. D. R. Bhat , E. V. Gotthelf , J. P. Halpern , Q. D. Wang , F. J. Lu , N. Mirabal

PSR J0108-1431 is a nearby, 170 Myr old, very faint radio pulsar near the "pulsar death line" in the P-Pdot diagram. We observed the pulsar field with the Chandra X-ray Observatory and detected a point source (53 counts in a 30 ks exposure,…

天体物理学 · 物理学 2009-06-23 G. G. Pavlov , O. Kargaltsev , J. A. Wong , G. P. Garmire

We report the discovery of a young and energetic pulsar in the Parkes multibeam survey of the Galactic plane. PSR J1016-5857 has a rotation period of 107 ms and period derivative of 8e-14, implying a characteristic age of 21 kyr and…

We report on a 19 ks observation of the pulsar J1016-5857 with the Chandra X-ray Observatory. This "Vela-like" pulsar has rotation period 107 ms, characteristic age 21 kyr, and spin-down power 2.6e36 ergs/s. A relatively bright centrally…

天体物理学 · 物理学 2009-11-10 F. Camilo , B. M. Gaensler , E. V. Gotthelf , J. P. Halpern , R. N. Manchester

The complex X-ray system IGR J11014-6103 (a.k.a. the Lighthouse nebula) is composed of a bow-shock pulsar wind nebula (PWN) as well as large-scale jet-like features, all launched by IGR J11014-6103 which is moving supersonically in the…

高能天体物理现象 · 物理学 2016-06-29 L. Pavan , G. Pühlhofer , P. Bordas , M. Audard , M. Balbo , E. Bozzo , D. Eckert , C. Ferrigno , M. D. Filipović , M. Verdugo , R. Walter

IGR J18483-0311 is a poorly known transient hard X-ray source discovered by INTEGRAL during observations of the Galactic Center region performed between 23--28 April 2003. Aims: To detect new outbursts from IGR J18483-0311 using INTEGRAL…

天体物理学 · 物理学 2009-11-13 V. Sguera , A. B. Hill , A. J. Bird , A. J. Dean , A. Bazzano , P. Ubertini , N. Masetti , R. Landi , A. Malizia , D. J. Clark , M. Molina

We report the discovery of PSR J2022+3842, a 24 ms radio and X-ray pulsar in the supernova remnant G76.9+1.0, in observations with the Chandra X-ray telescope, the Robert C. Byrd Green Bank Radio Telescope, and the Rossi X-ray Timing…

高能天体物理现象 · 物理学 2015-05-28 Z. Arzoumanian , E. V. Gotthelf , S. M. Ransom , S. Safi-Harb , R. Kothes , T. L. Landecker
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