Results 31 to 40 of about 1,910,738 (272)
The Astrophysical Journal, 2023 We report on the X-ray emission properties of the pulsar PSR J1849−0001 and its wind nebula (PWN), as measured by Chandra, XMM-Newton, NICER, Swift, and NuSTAR.
Chanho Kim +8 more
doaj +1 more source
AX J1910.7+0917: the slowest X-ray pulsar [PDF]
, 2017 Pulsations from the high-mass X-ray binary AX J1910.7+0917 were discovered during Chandra observations performed in 2011. We report here more details on this discovery and discuss the source nature.
L. Sidoli +18 more
semanticscholar +1 more source
Pulsars and X-Ray Sources [PDF]
Symposium - International Astronomical Union, 1973 We summarize some theoretical aspects of the X-ray emission from genuine pulsars and their relation to the more general problems of X-ray sources.
openaire +2 more sources
PROPELLER EFFECT IN THE TRANSIENT X-RAY PULSAR SMC X-2 [PDF]
, 2016 We report the results of the monitoring campaign of the transient X-ray pulsar SMC X-2 performed with the Swift/XRT telescope over the period of 2015 September–2016 January during the Type II outburst.
A. Lutovinov +4 more
semanticscholar +1 more source
Nuclear Physics B - Proceedings Supplements, 2004 We review the observational properties of the class of young neutron stars known as "anomalous X-ray pulsars," emphasizing the tremendous progress that has been made in recent years, and explain why these objects, like the "soft gamma repeaters," are today thought to be young, isolated, ultrahigh magnetic field neutron stars, or "magnetars."
Victoria M. Kaspi, Fotis P. Gavriil
openaire +3 more sources
Novel X-ray Communication Based XNAV Augmentation Method Using X-ray Detectors
Sensors, 2015 The further development of X-ray pulsar-based NAVigation (XNAV) is hindered by its lack of accuracy, so accuracy improvement has become a critical issue for XNAV.
Shibin Song +3 more
doaj +1 more source
The Orbit of the Binary X-Ray Pulsar 4U 1538−52 from [ITAL]Rossi X-Ray Timing Explorer[/ITAL] Observations [PDF]
, 2000 G. W. Clark
openalex +2 more sources
Spectral states in Be/X-ray pulsars [PDF]
Proceedings of An INTEGRAL view of the high-energy sky (the first 10 years) - 9th INTEGRAL Workshop and celebration of the 10th anniversary of the launch — PoS(INTEGRAL 2012), 2013 In the last quarter of a century, a unified characterization of the spectral evolution of low-mass X-ray binaries, both containing a neutron star and a black hole, was possible. In this context, the notion of source states characterizing the X-ray emission from black-hole binaries and neutron-star low-mass X-ray binaries revealed to be a very useful ...
Pablo Reig, E. Nespoli
openaire +3 more sources
REFINED NEUTRON STAR MASS DETERMINATIONS FOR SIX ECLIPSING X-RAY PULSAR BINARIES [PDF]
, 2011 We present an improved method for determining the mass of neutron stars in eclipsing X-ray pulsar binaries and apply the method to six systems, namely, Vela X-1, 4U 1538-52, SMC X-1, LMC X-4, Cen X-3, and Her X-1. In previous studies to determine neutron
M. Rawls +5 more
semanticscholar +1 more source
Discovery of an Energetic Pulsar Associated with SNR G76.9+1.0 [PDF]
, 2011 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 Explorer (RXTE). The
Arzoumanian, Z. +5 more
core +3 more sources