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Related papers: An extended X-ray object ejected from the PSR B125…

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We present observations with the Chandra X-ray Observatory of the pulsar wind nebula (PWN) within the supernova remnant G0.9+0.1. At Chandra's high resolution, the PWN has a clear axial symmetry; a faint X-ray point source lying along the…

Astrophysics · Physics 2009-11-06 B. M. Gaensler , M. J. Pivovaroff , G. P. Garmire

At least one massive binary system containing an energetic pulsar, PSR B1259-63/SS2883, has been recently detected in the TeV gamma-rays by the HESS telescopes. These gamma-rays are likely produced by particles accelerated in the vicinity…

Astrophysics · Physics 2009-11-13 Agnieszka Sierpowska-Bartosik , Wlodek Bednarek

We report the discovery of 0.59 s X-ray pulsations from the low-mass X-ray binary, 5.57 hr dipping and eclipsing ADC source 2A 1822-371. Pulse arrival time analysis indicates a circular orbit with e < 0.03 (95% confidence) and an asini for…

Astrophysics · Physics 2009-11-06 Peter G. Jonker , Michiel van der Klis

Recent X-ray polarimetric data on the prototypical black hole X-ray binary Cyg~X-1 from the Imaging X-ray Polarimetry Explorer present tight constraints on accretion geometry in the hard spectral state. Contrary to general expectations of a…

High Energy Astrophysical Phenomena · Physics 2023-05-31 Juri Poutanen , Alexandra Veledina , Andrei M. Beloborodov

We have detected weak soft X-ray emission from the Pulsar Wind Nebula trailing the high velocity star PSR 2224+65 (the `Guitar Nebula'). This X-ray flux gives evidence of \gamma~10^7 eV particles in the pulsar wind and constrains the…

Astrophysics · Physics 2009-10-30 Roger W. Romani , James M. Cordes , I. -A. Yadigaroglu

We present the results of a 50 ks long X-ray observation of the relativistic double pulsar system PSR J0737-3039 obtained with the XMM-Newton satellite in March 2004. The source has a soft spectrum (power law photon index = 3.5(+0.5,-0.3))…

Astrophysics · Physics 2009-11-10 A. Pellizzoni , A. De Luca , S. Mereghetti , A. Tiengo , F. Mattana , P. Caraveo , M. Tavani , G. F. Bignami

We report on a 95ks Chandra observation of the TeV emitting High Mass X-ray Binary LSI +61 303, using the ACIS-S camera in Continuos Clocking mode to search for a possible X-ray pulsar in this system. The observation was performed while the…

High Energy Astrophysical Phenomena · Physics 2015-05-18 N. Rea , D. F. Torres , M. van der Klis , P. G. Jonker , M. Mendez , A. Sierpowska-Bartosik

Aims: LS 5039 is an enigmatic high-mass gamma-ray binary which hosts a powerful O6.5V companion, but the nature of the compact object is still to be established using multi-wavelength observations. Methods: We analyzed phase-resolved…

High Energy Astrophysical Phenomena · Physics 2021-10-27 M. Falanga , A. M. Bykov , Z. Li , A. M. Krassilchtchikov , A. E. Petrov , E. Bozzo

We report Atacama Large Millimeter/submillimeter Array (ALMA) observations of the binary system containing the pulsar PSR B1259-63 orbiting around a Be star LS 2883 after the 2017 periastron passage. We detected radio continuum emission…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Yutaka Fujita , Akiko Kawachi , Takuya Akahori , Hiroshi Nagai , Masaki Yamaguchi

We report on the discovery of \geq 100 MeV {\gamma} rays from the binary system PSR B1259-63/LS 2883 using the Large Area Telescope (LAT) on board Fermi. The system comprises a radio pulsar in orbit around a Be star. We report on LAT…

High Energy Astrophysical Phenomena · Physics 2011-06-30 A. A. Abdo , Fermi LAT Collaboration , M. Chernyakova , A. Neronov , E. Grundstrom , the Fermi Pulsar Timing Consortium

We present X-ray imaging, timing, and phase resolved spectroscopy of the anomalous X-ray pulsar 1E 2259+58.6 using the Chandra X-ray Observatory. The spectrum is well described by a power law plus blackbody model with power law index =…

ASCA's long look at the 288 millisecond radio pulsar, PSR J0631+1036, reveals coherent X-ray pulsation from this source for the first time. The source was first detected in the serendipitous Einstein observation and later identified as a…

The recent discovery of a spectacular dust plume in the system 2XMM J160050.7-514245 (referred to as "Apep") suggested a physical origin in a colliding-wind binary by way of the "Pinwheel" mechanism. Observational data pointed to a…

Solar and Stellar Astrophysics · Physics 2020-10-13 Y. Han , P. G. Tuthill , R. M. Lau , A. Soulain , J. R. Callingham , P. M. Williams , P. A. Crowther , B. J. S. Pope , B. Marcote

We report on Chandra observations of the TeV emitting High Mass X-ray Binary LS 5039, for a total exposure of ~70ks, using the ACIS-S camera in Continuos Clocking mode to search for a possible X-ray pulsar in this system. We did not find…

Astrophysics of Galaxies · Physics 2015-05-28 N. Rea , D. F. Torres , G. A. Caliandro , D. Hadasch , M. van der Klis , P. G. Jonker , M. Mendez , A. Sierpowska-Bartosik

The source 4U 2206+54 is one of the most enigmatic high-mass X-ray binaries. In spite of intensive searches, X-ray pulsations have not been detected in the time range 0.001-1000 s. A cyclotron line at ~30 keV has been suggested by various…

Astrophysics · Physics 2009-11-13 P. Reig , J. M Torrejon , I. Negueruela , P. Blay , M. Ribo , J. Wilms

The detection of TeV gamma-rays from LS 5039 and the binary pulsar PSR B1259-63 by HESS, and from LS I +61 303 and the stellar-mass black hole Cygnus X-1 by MAGIC, provides a clear evidence of very efficient acceleration of particles to…

Astrophysics · Physics 2009-06-23 J. M. Paredes

We present in this paper the hard X-ray view of the pulsar wind nebula in G11.2-0.3 and its central pulsar PSR J1811-1925 as seen by NuSTAR. We complement the data with Chandra for a more complete picture and confirm the existence of a…

High Energy Astrophysical Phenomena · Physics 2020-03-04 K. K. Madsen , C. L. Fryer , B. W. Grefenstette , L. A. Lopez , S. Reynolds , A. Zoglauer

We report on the results of the extensive multi-wavelength campaign from optical to GeV gamma-rays of the 2014 periastron passage of PSR B1259-63, which is a unique high-mass gamma-ray emitting binary system with a young pulsar companion.…

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 address several issues regarding the interpretation of galactic \ggg-ray sources. We consider powerful pulsars in binaries producing X-ray and gamma-ray {\it unpulsed} emission from the shock interaction of relativistic pulsar winds with…

Astrophysics · Physics 2016-08-30 M. Tavani
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