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Related papers: Studying the $\gamma$-ray pulsar J1932+1916 and it…

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We present high resolution VLA images taken at the wavelengths of lambda 20 cm, lambda 6 cm, and lambda 3.6 cm in the vicinity of the pulsars PSR B1706-44 (PSR J1709-4428) and PSR B1643-43 (PSR J1646-4346). Both of these pulsars are young…

Astrophysics · Physics 2009-11-06 E. Giacani , D. A. Frail , W. M. Goss , M. Vieytes

We present a Chandra X-ray observation of G12.82-0.02, a shell-like radio supernova remnant coincident with the TeV gamma-ray source HESS J1813-178. We resolve the X-ray emission from the co-located ASCA source into a compact object…

Astrophysics · Physics 2008-11-26 E. V. Gotthelf , D. J. Helfand

We report the detection of extended emission around the anomalous X-ray pulsar AXP 1E1547.0-5408 using archival data of the Chandra X-ray satellite. The extended emission consists of an inner part, with an extent of 45arsec and an outer…

High Energy Astrophysical Phenomena · Physics 2014-11-20 Jacco Vink , Aya Bamba

We present radio observations of a region in the vicinity of the young pulsar PSR B1853+01 in the supernova remnant W44. The pulsar is located at the apex of an extended feature with cometary morphology. We argue on the basis of its…

Astrophysics · Physics 2009-10-28 D. A. Frail , E. B. Giacani , W. M. Goss , G. Dubner

We present the results of detailed spatial and spectral analysis of the pulsar wind nebula (PWN) in supernova remnant Kes 75 (G29.7-0.3) using a deep exposure with Chandra X-ray observatory. The PWN shows a complex morphology with clear…

Astrophysics · Physics 2009-11-13 C. -Y. Ng , P. O. Slane , B. M. Gaensler , J. P. Hughes

We report on X-ray studies of the gamma-ray pulsar PSR J1418$-$6058 in the Rabbit pulsar wind nebula (PWN) carried out using archival Chandra and XMM-Newton observations. A refined timing analysis performed with the 120-ks XMM-Newton data…

High Energy Astrophysical Phenomena · Physics 2020-03-25 Minjun Kim , Hongjun An

We present spectral and timing analyses of the X-ray emission from the pulsar wind nebula DA 495 and its central object, J1952.2+2925, suggested to be the pulsar, using archival Chandra and XMM-Newton data. J1952.2+2925 has a pure thermal…

High Energy Astrophysical Phenomena · Physics 2015-12-14 A. Karpova , D. Zyuzin , A. Danilenko , Yu. Shibanov

We observed the young energetic pulsar J1617-5055 with the Chandra ACIS detector for 60 ks. In addition to the pulsar, the X-ray images show a faint pulsar-wind nebula (PWN) seen up to ~1' from the pulsar. Deconvolution and reconstruction…

Astrophysics · Physics 2015-05-13 O. Kargaltsev , G. G. Pavlov , J. A. Wong

We present a Chandra X-ray observation of the very high energy $\gamma$-ray source HESS$ $J1640-465. We identify a point source surrounded by a diffuse emission that fills the extended object previously detected by XMM Newton at the…

High Energy Astrophysical Phenomena · Physics 2014-11-20 A. Lemiere , P. Slane , B. M. Gaensler , S. Murray

We report the results of a 50 ks Chandra observation of the recently discovered radio object G141.2+5.0, presumed to be a pulsar-wind nebula. We find a moderately bright unresolved X-ray source which we designate CXOU J033712.8 615302…

High Energy Astrophysical Phenomena · Physics 2016-01-20 Stephen P. Reynolds , Kazimierz J. Borkowski

We report on sensitive new 1.4-GHz VLA radio observations of the pulsar wind nebula G21.5-0.9, powered by PSR J1833-1034, and its environs. Our observations were targeted at searching for the radio counterpart of the shell-like structure…

Astrophysics of Galaxies · Physics 2015-05-19 Michael F. Bietenholz , Heather Matheson , Samar Safi-Harb , Crystal Brogan , Norbert Bartel

We observed the pulsar PSR J1648-4611 with Suzaku. Two X-ray sources, Suzaku J1648-4610 (Src A) and Suzaku J1648-4615 (Src B), were found in the field of view. Src A is coincident with the pulsar PSR J1648-4611, which was also detected by…

High Energy Astrophysical Phenomena · Physics 2015-06-12 Michito Sakai , Hironori Matsumoto , Yoshito Haba , Yasufumi Kanou , Youhei Miyamoto

We present a deep observation with the X-ray Multi-Mirror Mission of PSR B1823-13, a young pulsar with similar properties to the Vela pulsar. We detect two components to the X-ray emission associated with PSR B1823-13: an elongated core of…

Astrophysics · Physics 2009-11-07 Bryan Gaensler , Norbert Schulz , Vicky Kaspi , Michael Pivovaroff , Werner Becker

We present a catalog of 34 diffuse features identified in X-ray images of the Galactic center taken with the Chandra X-ray Observatory. Several of the features have been discussed in the literature previously, including 7 that are…

Astrophysics · Physics 2009-11-13 M. P. Muno , F. K. Baganoff , W. N. Brandt , M. R. Morris , J. -L. Starck

We analyze new XMM-Newton and archival Chandra observations of the middle-aged $\gamma$-ray radio-quiet pulsar J1957+5033. We detect, for the first time, X-ray pulsations with the pulsar spin period of the point-like source coinciding by…

High Energy Astrophysical Phenomena · Physics 2022-06-09 D. A. Zyuzin , A. V. Karpova , Y. A. Shibanov , A. Y. Potekhin , V. F. Suleimanov

Based on a Chandra ACIS observation, we report the detection of an extended X-ray feature close to the center of the remnant DA 530 with 5.3 sigma above the background within a circle of 20'' radius. This feature, characterized by a…

Astrophysics · Physics 2009-11-13 Bing Jiang , Yang Chen , Q. Daniel Wang

A Chandra observation of the isolated hard X-ray source XMMU J061804.3+222732, located in the region of apparent interaction of the supernova remnant IC 443 with a molecular cloud, resolved the complex structure of the source in a few…

Astrophysics · Physics 2009-11-10 A. M. Bykov , F. Bocchino , G. G. Pavlov

Using the Chandra X-ray Observatory we have discovered a diffuse, center-filled region of hard X-ray emission within the young, oxygen-rich supernova remnant (SNR) G292.0+1.8. Near the peak of this diffuse emission lies a point-like source…

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…

High Energy Astrophysical Phenomena · Physics 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

The young and energetic pulsar B1509-58 powers a bright X-ray synchrotron nebula, embedded in the unusual supernova remnant G320.4-1.2. We present observations of this system with the Chandra X-ray Observatory, which show a spectacularly…

Astrophysics · Physics 2007-05-23 B. M. Gaensler , J. Arons , M. J. Pivovaroff , V. M. Kaspi