English
Related papers

Related papers: Observations of the $\gamma$-ray pulsar J1932+1916…

200 papers

We report on the results of Chandra X-ray observations of the $\gamma$-ray radio-quiet pulsar J1932+1916. We confirm the previous detection of the pulsar counterpart and its pulsar wind nebula in X-rays from low spatial resolution data…

High Energy Astrophysical Phenomena · Physics 2020-03-02 O. D. Medvedev , A. V. Karpova , Yu. A. Shibanov , D. A. Zyuzin , G. G. Pavlov

A largely extended X-ray emission was discovered around the pulsar PSR J1357-6429 with the Suzaku deep observations. The pulsar, whose characteristic age is 7.3 kyr, is located within the TeV gamma-ray source HESS J1356-645. The extended…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Masaharu Izawa , Tadayasu Dotani , Takahisa Fujinaga , Aya Bamba , Masanobu Ozaki , Junko S Hiraga

Using archival X-ray data we have found point-like X-ray counterpart candidates positionally coincident with six $\gamma$-ray pulsars discovered recently in the Fermi Gamma-ray Space Telescope data by the Einstein@Home project. The…

High Energy Astrophysical Phenomena · Physics 2018-02-13 Dmitry A. Zyuzin , Anna V. Karpova , Yura A. Shibanov

We report on diffuse X-ray emission associated with the nearby solitary millisecond pulsar PSR J2124-3358 detected with XMM-Newton and Chandra. The emission extends from the pulsar to the northwest by ~0.5 arcmin. The spectrum of the…

Astrophysics · Physics 2009-11-11 C. Y. Hui , W. Becker

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 obtained six observations of PSR J1741-2054 using the $Chandra$ ACIS-S detector totaling $\sim$300 ks. By registering this new epoch of observations to an archival observation taken 3.2 years earlier using X-ray point sources in the…

We have discovered an extended X-ray feature which is apparently associated with millisecond pulsar (MSP) PSR J1911-1114 from a XMM-Newton observation, which extends for ~1' and the radio timing position of PSR J1911-1114 is in the mid…

High Energy Astrophysical Phenomena · Physics 2018-12-26 Jongsu Lee , C. Y. Hui , J. Takata , L. C. C. Lin

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,…

Astrophysics · Physics 2009-06-23 G. G. Pavlov , O. Kargaltsev , J. A. Wong , G. P. Garmire

Using the Chandra X-ray Observatory, we have pinpointed the location of a faint X-ray point source (CXOUJ182913.1-125113) and an associated diffuse nebula in the composite supernova remnant G18.95-1.1. These objects appear to be the…

High Energy Astrophysical Phenomena · Physics 2015-05-19 R. Tuellmann , P. P. Plucinsky , T. J. Gaetz , P. Slane , J. P. Hughes , I. Harrus , T. G. Pannuti

We present results of investigation of the poorly studied X-ray pulsar Swift J1816.7--1613 during its transition from the type I outburst to the quiescent state. Our studies are based on the data obtained from X-ray observatories…

We present the first X-ray detection of the very young pulsar PSR J1357-6429 (characteristic age of 7.3 kyr) using data from the XMM-Newton and Chandra satellites. We find that the spectrum is well described by a power-law plus blackbody…

Astrophysics · Physics 2009-02-23 P. Esposito , A. Tiengo , A. De Luca , F. Mattana

We used optical images taken with the Very Large Telescope (VLT) in the B and V bands to search for the optical counterpart of PSR J1028-5819 or constrain its optical brightness. At the same time, we used an archival Suzaku observation to…

High Energy Astrophysical Phenomena · Physics 2015-06-05 R. P. Mignani , M. Razzano , P. Esposito , A. De Luca , M. Marelli , S. R. Oates , P. Saz-Parkinson

We report the results of a deep XMM-Newton observation of the radio-faint $\gamma$-ray pulsar J1741-2054 and its nebula together with the analysis of 5 years of Fermi LAT data. The X-ray spectrum of the pulsar is consistent with an absorbed…

High Energy Astrophysical Phenomena · Physics 2015-06-19 M. Marelli , A. Belfiore , P. Saz Parkinson , P. Caraveo , A. De Luca , C. Sarazin , D. Salvetti , G. R. Sivakoff , F. Camilo

We observed the brightest part of HESS J1825-137 with the Suzaku XIS, and found diffuse X-rays extending at least up to 15' (~ 17 pc) from the pulsar PSR J1826-1334. The spectra have no emission line, and are fitted with an absorbed…

Astrophysics · Physics 2015-05-13 H. Uchiyama , H. Matsumoto , T. G. Tsuru , K. Koyama , A. Bamba

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 present X-ray observations of the "redback" eclipsing radio millisecond pulsar and candidate radio pulsar/X-ray binary transition object PSR J1723-2837. The X-ray emission from the system is predominantly non-thermal and exhibits…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Slavko Bogdanov , Paolo Esposito , Fronefield Crawford , Andrea Possenti , Maura A. McLaughlin , Paulo Freire

We used the 10.4m Gran Telescopio Canarias to search for the optical counterparts to four isolated $\gamma$-ray pulsars, all detected in the X-rays by either \xmm\ or \chan\ but not yet in the optical. Three of them are middle-aged pulsars…

High Energy Astrophysical Phenomena · Physics 2018-05-02 R. P. Mignani , V. Testa , N. Rea , M. Marelli , D. Salvetti , D. Torres , E. de Ona Wilhelmi

We present the results obtained from timing and spectral studies of the newly discovered accreting X-ray binary pulsar Swift J0243.6+6124 using a NuSTAR observation in 2017 October at a flux level of ~280 mCrab. Pulsations at 9.85423(5) s…

High Energy Astrophysical Phenomena · Physics 2017-11-30 Gaurava K. Jaisawal , Sachindra Naik , J. Chenevez

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…

Astrophysics · Physics 2009-11-10 F. Camilo , B. M. Gaensler , E. V. Gotthelf , J. P. Halpern , R. N. Manchester

We present XMM-Newton and Chandra X-ray observations of the middle-aged radio pulsar PSR B0355+54. Our X-ray observations reveal emission not only from the pulsar itself, but also from a compact diffuse component extending ~50'' in the…

‹ Prev 1 2 3 10 Next ›