Results 61 to 70 of about 547,290 (394)
A window into the neutron star: Modelling the cooling of accretion heated neutron star crusts [PDF]
In accreting neutron star X-ray transients, the neutron star crust can be substantially heated out of thermal equilibrium with the core during an accretion outburst.
Ootes, L. S.+4 more
core +5 more sources
The plant-microbial interactive relations with respect to determination of the mycoflora of the Castanea sativa Mill. nuts, crust, leaves and pollen and their effect on the host organism in four Slovak regions were studied.
Miroslava Kačániová+4 more
doaj +1 more source
Late time cooling of neutron star transients and the physics of the inner crust [PDF]
An accretion outburst onto a neutron star transient heats the neutron star's crust out of thermal equilibrium with the core. After the outburst the crust thermally relaxes toward equilibrium with the neutron star core and the surface thermal emission powers the quiescent X-ray light curve.
arxiv +1 more source
Non-radial Oscillation Modes of Compact Stars with a Crust [PDF]
Oscillation modes of isolated compact stars can, in principle, be a fingerprint of the equation of state (EoS) of dense matter. We study the non-radial high-frequency l=2 spheroidal modes of neutron stars and strange quark stars, adopting a two-component
Flores, C. Vasquez+2 more
core +3 more sources
Copper sulfide based electrocatalysts for CO2 conversion are selective for production of formate as major product. Transformations under electrochemical conditions result in significant sulfur loss, and this study examines the nature of how persistent, residual sulfur (observed as surface SO42– species and S dissolved in the electrolyte) can sustain ...
Sasho Stojkovikj+8 more
wiley +1 more source
Crust effects and the cooling relaxation time in highly magnetized neutron stars [PDF]
We study the effects of high magnetic fields on the structure and on the geometry of the crust in neutron stars. We find that the crust geometry is substantially modified by the magnetic field inside the star. We build stationary and axis-symmetric magnetized stellar models by using well-known equations of state to describe the neutron star crust ...
arxiv +1 more source
Quiescent thermal emission from neutron stars in LMXBs [PDF]
We monitored the quiescent thermal emission from neutron stars in low-mass X-ray binaries after active periods of intense activity in x-rays (outbursts).
Aguilera, Deborah N.+2 more
core +3 more sources
10 Years Development of Potassium‐Ion Batteries
Significant progress is made in PIBs over the past decade, but the improvements based on half‐cell testing, low mass loading, and low energy density are insufficient for practical applications. This review summarizes the challenges and strategies for PIBs, highlights the importance of further research focusing on full cells, and provides an analysis of
Mingnan Li+7 more
wiley +1 more source
Research subject. The relative deformation of rock masses, which was obtained in the Urals at depths below500 m, i.e. below the zone of massif disintegration, through the use of traditional geodetic measurement methods, allows correction of the results ...
A. V. Zubkov+2 more
doaj +1 more source