Results 161 to 170 of about 53,868 (337)
The Discovery of Two Quadruple Star Systems with the Second and Third Shortest Outer Periods
We present the discovery of two quadruple star systems—TIC 285853156 and TIC 392229331—each consisting of two bound eclipsing binary stars. Among the most compact quadruples known, TIC 392229331 and TIC 285853156 have the second and third shortest outer ...
Brian P. Powell +14 more
doaj +1 more source
Strongly interacting matter exhibits deconfined behavior in massive neutron stars. [PDF]
Annala E +6 more
europepmc +1 more source
Orbital evolution of potentially habitable planets of tidally interacting binary stars [PDF]
David E. Graham +2 more
openalex +1 more source
This work addresses the challenge of current–voltage asymmetry in scalable laminated semitransparent organic photovoltaics (OPVs) for indoor applications. Vertical stratification of materials is shown to create an energy barrier, leading to performance differences under different illumination directions.
Gulzada Beket +15 more
wiley +1 more source
GANBISS: a new GPU accelerated N-body code for binary star systems. [PDF]
Zimmermann M, Pilat-Lohinger E.
europepmc +1 more source
500 - 3200 Å Observations of the Interacting Binary Stars V356 Sgr and β Lyr [PDF]
R. S. Polidan
openalex +1 more source
The study develops elastin–fibrin scaffolds and evaluates angiogenesis using the chorioallantoic membrane (CAM) model. Advanced imaging with confocal microscopy and Indocyanine Green dye enables precise 3D quantification of vascular networks. Findings demonstrate superior microvessel visualization compared to micro‐CT using Microfil and Optiray 350 ...
Ece Melis Er +8 more
wiley +1 more source
Electrodynamics and Dissipation in the Binary Magnetosphere of Premerger Neutron Stars
We investigate the energy release in the interacting magnetospheres of binary neutron stars (BNSs) with global 3D force-free electrodynamics simulations.
Jens F. Mahlmann, Andrei M. Beloborodov
doaj +1 more source
Exploring the Variability of Three Be Stars with TESS Observations
Be stars are rapidly rotating B-type stars surrounded by circumstellar disks formed from self-ejected material. Understanding the mechanisms driving mass ejection and disk formation, known as the Be phenomenon, requires a detailed investigation of their ...
Laerte Andrade +3 more
doaj +1 more source

