X-RAY OBSERVATIONS OF BLACK WIDOW PULSARS [PDF]
The Astrophysical Journal, 2014 8 pages, 6 figures, 2 tables, submitted to ...
Paul S. Ray +10 more
openaire +5 more sources
X-ray and $\gamma$-ray Studies of the Millisecond Pulsar and Possible X-ray Binary/Radio Pulsar Transition Object PSR J1723-2837 [PDF]
, 2013 We present X-ray observations of the "redback" eclipsing radio millisecond pulsar and candidate radio pulsar/X-ray binary transition object PSR J1723-2837.
Bogdanov, Slavko +5 more
core +3 more sources
On the soft emission mechanism in X-ray pulsars
Journal of Theoretical and Applied Physics, 2019 We propose a mechanism responsible for the soft emission in X-ray pulsars. We discuss the origin of the soft emission for isolated X-ray pulsars as well as for soft gamma-ray repeaters and anomalous X-ray pulsars.
Paolo Cea
doaj +1 more source
Exploring the Extra Component in the Gamma-ray Emission of the New Redback Candidate 3FGL J2039.6-5618 [PDF]
Journal of Astronomy and Space Sciences, 2016 A redback system is a binary system composed of a pulsar and a main sequence star. The inverse Compton (IC) scattering between the stellar soft photons and the relativistic pulsar wind will generate orbital-modulating GeV photons.
Cho-Wing Ng +2 more
doaj +1 more source
THE DUST-SCATTERING X-RAY RINGS OF THE ANOMALOUS X-RAY PULSAR 1E 1547.0–5408 [PDF]
, 2009 On 2009 January 22 numerous strong bursts were detected from the anomalous X-ray pulsar 1E 1547.0–5408. Swift/XRT and XMM-Newton/EPIC observations carried out in the following two weeks led to the discovery of three X-ray rings centered on this source ...
A. Tiengo +19 more
semanticscholar +1 more source
EVOLUTION OF THE X-RAY PROFILE OF THE CRAB PULSAR [PDF]
The Astrophysical Journal, 2016 ABSTRACT Using the archival data from the Rossi X-ray Timing Explorer, we study the evolution of the Crab pulsar’s X-ray profile in a time span of 11 years. The X-ray profiles, as characterized by a few parameters, changed slightly, but with high statistical significance in these years: the separation of the two peaks increased with a ...
M. Y. Ge +7 more
openaire +4 more sources
A new nearby pulsar wind nebula overlapping the RX J0852.0-4622 supernova remnant [PDF]
, 2012 Energetic pulsars can be embedded in a nebula of relativistic leptons which is powered by the dissipation of the rotational energy of the pulsar.
Acero, F. +4 more
core +4 more sources
X-Ray Studies of the Pulsar PSR J1420–6048 and Its TeV Pulsar Wind Nebula in the Kookaburra Region
The Astrophysical Journal, 2023 We present a detailed analysis of broadband X-ray observations of the pulsar PSR J1420−6048 and its wind nebula (PWN) in the Kookaburra region with Chandra, XMM-Newton, and NuSTAR.
Jaegeun Park +6 more
doaj +1 more source
Discovery of a prominent cyclotron absorption feature from the transient X-ray pulsar X0331+53
, 1990 A remarkable absorption feature at 28.5 keV, attributable to electron cyclotron resonance, has been discovered in the 1.9-60-keV X-ray spectrum of the recurrent transient X-ray pulsar X0331 + 53.
K. Makishima +17 more
semanticscholar +1 more source
Discovery of Radio Pulsations from the X-Ray Pulsar J0205+6449 in Supernova Remnant 3C 58 with the Green Bank Telescope [PDF]
, 2002 We report the discovery with the 100 m Green Bank Telescope of 65 ms radio pulsations from the X-ray pulsar J0205+6449 at the center of supernova remnant 3C 58, making this possibly the youngest radio pulsar known. From our observations at frequencies of
F. Camilo +17 more
semanticscholar +1 more source