Results 131 to 140 of about 25,195 (313)
The recent discovery of planetesimals orbiting white dwarfs has renewed interest in the final chapters of the evolution of planetary systems. Although observational and theoretical studies have examined the dynamical evolution of these systems, studies ...
Matthew Route
doaj +1 more source
Serendipitous identifications of two magnetic white dwarfs [PDF]
N. Achilleos +2 more
openalex +1 more source
The donor star radial velocity curve in the cataclysmic variable GY Cnc confirms white dwarf eclipse modelling mass [PDF]
S. P. Littlefair +4 more
openalex +1 more source
Physically consistent mesoscale model evaluation in complex terrain
This study introduces a novel approach for evaluating mesoscale atmospheric models in complex terrain by selecting physically consistent grid points and applying height‐based corrections. The method corrects for sensor height and terrain elevation differences between model and observations using a time‐varying lapse rate.
Gaspard Simonet +2 more
wiley +1 more source
In recent years, the gauge group U 1 L μ − L τ $$ \textrm{U}{(1)}_{L_{\mu }-{L}_{\tau }} $$ has received a lot of attention since it can, in principle, account for the observed excess in the anomalous muon magnetic moment (g − 2) μ , as well as the ...
Patrick Foldenauer, Jaime Hoefken Zink
doaj +1 more source
Hubble COS Spectroscopy of the Dwarf Nova CW Mon: The White Dwarf in Quiescence? [PDF]
Hause C +6 more
europepmc +1 more source
Constraining Effective Temperature, Mass and Radius of Hot White Dwarfs [PDF]
Elvis do A. Soares
openalex +1 more source
Loss Behavior in Supervised Learning With Entangled States
Entanglement in training samples supports quantum supervised learning algorithm in obtaining solutions of low generalization error. Using analytical as well as numerical methods, this work shows that the positive effect of entanglement on model after training has negative consequences for the trainability of the model itself, while showing the ...
Alexander Mandl +4 more
wiley +1 more source
Shocking and Mass Loss of Compact Donor Stars in Type Ia Supernovae
Type Ia supernovae arise from thermonuclear explosions of white dwarfs accreting from a binary companion. Following the explosion, the surviving donor star leaves at roughly its orbital velocity.
Tin Long Sunny Wong +2 more
doaj +1 more source

