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21 papers · 2 filters
Sub-arcminute localization of 13 repeating fast radio bursts detected by CHIME/FRB
Daniele Michilli, Mohit Bhardwaj, Charanjot Brar +23
We report on improved sky localizations of thirteen repeating fast radio bursts (FRBs) discovered by CHIME/FRB via the use of interferometric techniques on channelized voltages fro…
Constraints on neutron star superfluidity from the cooling neutron star in Cassiopeia A using all Chandra ACIS-S observations
Peter S. Shternin, Dmitry D. Ofengeim, Craig O. Heinke +1
Analysis of Chandra observations of the neutron star (NS) in the centre of the Cassiopeia A supernova remnant taken in the subarray (FAINT) mode of the ACIS detector performed by P…
Inside the core of a young massive star cluster: 3D MHD simulations
D. V. Badmaev, A. M. Bykov, M. E. Kalyashova
Young massive star clusters inhabit regions of star formation and play an essential role in the galactic evolution. They are sources of both thermal and non-thermal radiation, and…
Neutron star inner crust: reduction of shear modulus by nuclei finite size effect
Nikita A. Zemlyakov, Andrey I. Chugunov
The elasticity of neutron star crust is important for adequate interpretation of observations. To describe elastic properties one should rely on theoretical models. The most widely…
XMM-Newton observations of PSR J0554+3107: pulsing thermal emission from a cooling high-mass neutron star
A. S. Tanashkin, A. V. Karpova, A. Y. Potekhin +2
XMM-Newton observations of the middle-aged radio-quiet -ray pulsar J0554+3107 allowed us, for the first time, firmly identify it in X-rays by detection of pulsations with the pu…
Neutron star crust in Voigt approximation II: general formula for electron screening correction for effective shear modulus
Andrey I. Chugunov
The main contribution to the effective shear modulus of neutron star crust can be calculated within Coulomb solid model and can be approximated by simple analytical expression for…