Results 91 to 100 of about 1,421,542 (340)
Multimessenger Bayesian parameter inference of a binary neutron star merger [PDF]
The combined detection of a binary neutron star merger in both gravitational waves (GWs) and electromagnetic (EM) radiation spanning the entire spectrum – GW170817/AT2017gfo/GRB170817A – marks a breakthrough in the field of multimessenger astronomy ...
M. Coughlin+3 more
semanticscholar +1 more source
ABSTRACT Objective Prognostication of disease course and prediction of treatment response in multiple sclerosis is an unmet need. We compared the performance of serum neurofilament light chain Z scores (age‐ and BMI‐adjusted) with absolute concentrations for the prediction of response to disease‐modifying therapy.
Maximilian Einsiedler+43 more
wiley +1 more source
Delayed and Displaced: The Impact of Binary Interactions on Core-collapse SN Feedback
Core-collapse supernova feedback models in hydrodynamical simulations typically assume that all stars evolve as single stars. However, the majority of massive stars are formed in binaries and multiple systems, where interactions with a companion can ...
Tom Wagg+9 more
doaj +1 more source
Nearly a hundred binary black holes (BBHs) have been discovered with gravitational-wave signals emitted at their merging events. Thus, it is quite natural to expect that significantly more abundant BBHs with wider separations remain undetected in the ...
Toshinori Hayashi+2 more
doaj +1 more source
Can we distinguish low mass black holes in neutron star binaries?
The detection of gravitational waves from coalescing binary neutron stars represents another milestone in gravitational-wave astronomy. However, since LIGO is currently not as sensitive to the merger/ringdown part of the waveform, the possibility that ...
East, William E.+2 more
core +1 more source
Thermal Timescale Mass Transfer Rates in Intermediate-Mass X-ray Binaries [PDF]
Thermal timescale mass transfer generally occurs in close binaries where the donor star is more massive than the accreting star. The mass transfer rates are usually estimated in terms of the Kelvin-Helmholtz timescale of the donor star.
Li, Xiang-Dong, Xu, Xiao-Jie
core +1 more source
Eccentric Black Hole Mergers in Dense Star Clusters: The Role of Binary–Binary Encounters [PDF]
We present the first systematic study of strong binary–single and binary–binary black hole (BH) interactions with the inclusion of general relativity.
M. Zevin+4 more
semanticscholar +1 more source
The rs10191329 Risk Allele Is Associated With Pronounced Retinal Layer Atrophy in Multiple Sclerosis
ABSTRACT Objective To investigate whether the rs10191329 risk allele in the DYSF–ZNF638 locus, which is implicated in central nervous system resilience rather than immune‐mediated pathology, is associated with retinal layer thinning, a biomarker of neuroaxonal damage in relapsing multiple sclerosis (RMS). Methods From a prospective observational study,
Gabriel Bsteh+22 more
wiley +1 more source
Binary Star Orbits. VI. The Interferometric-spectroscopic Binary 73 Leo
Discordances in radial-velocity measurements of 73 Leonis, made more than a century ago, gave rise to the first suggestion that this fifth-magnitude star was a binary system, but it was 40 yr before an accurate investigation of the object commenced, and ...
Brian D. Mason+9 more
doaj +1 more source
Optical Properties and Variability of the Be X-Ray Binary CPD-29 2176
Be X-ray binaries (Be XRBs) are high-mass X-ray binaries, with a neutron star or black hole orbiting and accreting material from a nonsupergiant B-star that is rotating at a near critical rate.
Clarissa M. Pavao+4 more
doaj +1 more source