Results 41 to 50 of about 427 (123)
Noisy Timing Behavior is a Feature of Central Compact Object Pulsars
We present a timing study of the three known central compact object (CCO) pulsars, isolated cooling neutron stars in supernova remnants, using observations from Chandra, XMM-Newton, and NICER spanning two decades.
K. I. Perez +2 more
doaj +1 more source
Single-crystal diamond stands out among all the candidate materials that could be exploited to fabricate compound refractive lenses (CRLs) owing to its extremely stable properties. Among all related experimental features, beam divergence, χ-angles relative to the incoming beam in Eulerian geometry and different positions of the X-ray beam relative to ...
Qiuyuan Zhang +8 more
openaire +2 more sources
A Pulse Profile Change Possibly Associated with a Glitch in the Anomalous X‐Ray Pulsar 4U 0142+61
14 pages, 4 figures, accepted by ...
Morii, M., Kawai, N., Shibazaki, N.
openaire +2 more sources
Physics of Neutron Star Crusts
The physics of neutron star crusts is vast, involving many different research fields, from nuclear and condensed matter physics to general relativity.
Chamel Nicolas, Haensel Pawel
doaj
A Giant Glitch in the Energetic 69 ms X-ray Pulsar AXS J161730-505505
We present new results on the recently discovered 69 ms X-ray pulsar AXS J161730-505505, the sixth youngest sample of all known pulsars. We have undertaken a comprehensive X-ray observing campaign of AXS J161730-505505 with the ASCA, SAX, and XTE observatories and follow its long term spin-down history between 1989 and 1999, using these, archival GINGA
Torii, K. +4 more
openaire +2 more sources
Simulations of the periods, split regularities and mirror symmetries of the glitch pattern of a Si(111) crystal along with the azimuthal angles are presented. The glitch patterns of Si(111) double-crystal monochromators (DCMs) are found to be the superposition of the two sets of glitch patterns from the two crystals.
Zheng, Tang +6 more
openaire +2 more sources
We present 7 eclipse timings of the low mass X-ray binary EXO0748-676 obtained with the USA experiment during 1999-2000 as well as 122 eclipse timings obtained with RXTE during 1996-2000. According to our analysis, the mean orbital period has increased by ~8 ms between the pre-RXTE era (1985-1990) and the RXTE/USA era (1996-2000).
Wolff, M. T. +4 more
openaire +2 more sources
A hybrid GNA instability. [PDF]
Karmakar PK, Kalita D, Atteya A.
europepmc +1 more source
Wiggler radiation at a low-emittance storage ring and its usage for X-ray absorption spectroscopy. [PDF]
Klementiev K, Tarawneh H, Tavares PF.
europepmc +1 more source
Revolutionizing Orthopedic Healthcare: The Role of Robotics. [PDF]
Ram PR +4 more
europepmc +1 more source

