Results 41 to 50 of about 43,788 (263)
Multi-wavelength studies of the gamma-ray pulsar PSR J1907+0602
, 2012 PSR J1907+0602 is a radio-faint, 107-ms GeV gamma-ray pulsar that was discovered with the Fermi LAT in a blind pulsar search. PSR J1907+0602 is located near the bright, extended TeV gamma-ray source MGRO J1908+06 which may be an associated pulsar wind ...
Pandel, Dirk, Scott, Robert
core +1 more source
Analysing X-ray pulsar profiles [PDF]
Astronomy & Astrophysics, 2012 Aims. By analysing the asymmetric pulse profiles of the transient Be/X-ray binaries 4U 0115+63 and V 0332+53 we aim to identify the origin of the pulsed emission to understand the geometry of the accretion onto the neutron star. Methods. We have applied the pulse-profile decomposition method, which enabled us to find two symmetric pulse profiles for ...
M. Sasaki +4 more
openaire +1 more source
Probing the Pulsar Wind Nebula of PSR B0355+54 [PDF]
, 2006 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 opposite direction
Becker W. +9 more
core +2 more sources
AIP Conference Proceedings, 2001 The observational properties of the six known Anomalous X-ray Pulsars are described in the context of the main theoretical models for this enigmatic class of objects.
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Nuclear-Powered X-ray Millisecond Pulsars
, 2021 Nuclear-powered X-ray millisecond pulsars are the third type of millisecond pulsars, which are powered by thermonuclear fusion processes. The corresponding brightness oscillations, known as burst oscillations, are observed during some thermonuclear X-ray bursts, when the burning and cooling accreted matter gives rise to an azimuthally asymmetric ...
openaire +2 more sources
Applied SciencesPulsars are neutron stars with high rotation speeds and have extraordinary long-term rotational stability. X-ray pulsar-based navigation (XNAV) is a navigation method that estimates the position and velocity of a spacecraft using the X-ray radiation from
Kun Jiang +3 more
doaj +1 more source
XMM-Newton observations of PSr B1259-63 near the 2004 periastron passage
, 2006 PSR B1259-63 is in a highly eccentric 3.4 year orbit with a Be star and crosses the Be star disc twice per orbit, just prior to and just after periastron.
Chernyakova, M. +4 more
core +1 more source
Comprehensive Measurement of Position and Velocity in the Transverse Direction Using the Crab Pulsar
AerospaceTraditional X-ray pulsar ranging and velocity measurement methods only estimate the radial position and velocity information of the pulsar. For non-linear orbits, errors in the transverse position and velocity of the pulsar lead to errors in the radial ...
Yuan Feng +4 more
doaj +1 more source
Young Crab-like pulsars and luminous X-ray sources in starbursts and optically dull galaxies
, 2004 Recent Chandra observations of nearby galaxies have revealed a number of ultraluminous X-ray sources (ULXs) with super-Eddington luminosities, away from the central regions of non-active galaxies. The nature of these sources is still debated.
Becker W. +8 more
core +2 more sources
Radio-quiet and radio-loud pulsars: similar in Gamma-rays but different in X-rays [PDF]
, 2015 We present new Chandra and XMM-Newton observations of a sample of eight radio-quiet Gamma-ray pulsars detected by the Fermi Large Area Telescope. For all eight pulsars we identify the X-ray counterpart, based on the X-ray source localization and the best
De Luca, A. +6 more
core +3 more sources