Results 161 to 170 of about 116,321 (322)
Mapping Stellar Surfaces. I. Degeneracies in the Rotational Light-curve Problem
Rodrigo Luger +3 more
openalex +1 more source
Recovery of TESS Stellar Rotation Periods with Deep Learning [PDF]
Zachary R. Claytor +5 more
openalex +1 more source
A two‐step approach combining laser powder bed fusion of FeSi electrical steel with Bakelite infiltration enables the fabrication of multifunctional gyroid lattice composites. The resulting structures exhibit high strength, magnetic anisotropy, and complete polymer infiltration, demonstrating a simple and scalable route toward lightweight, mechanically
Angelo F. Andreoli +9 more
wiley +1 more source
Measuring the magnetic fields in the chromospheres of low-mass stars. [PDF]
Cang T +13 more
europepmc +2 more sources
The work demonstrates that strategic wall‐thickness grading in diamond triply periodic minimal surface lattices enables precise tuning of deformation and failure behavior under compression. Different gradation patterns guide how and where the structure collapses, improving energy absorption or promoting controlled brittle failure.
Giovanni Rizza +3 more
wiley +1 more source
Metal-enriched Pair-instability Supernovae: Effects of Rotation
In this paper, we revisit metal-enriched rotating pair-instability supernovae (PISNe) models for metallicities consistent with the Small Magellanic Cloud, the Large Magellanic Cloud (LMC), and 0.1 Z _⊙ .
Hideyuki Umeda, Chris Nagele
doaj +1 more source
Signature of non-isotropic distribution of stellar rotation inclination angles in the Praesepe cluster [PDF]
Geza Kovacs
openalex +1 more source
In this study, the interplay of dipolar dynamics and ionic charge transport in MOF compounds is investigated. Synthesizing the novel structure CFA‐25 with integrated freely rotating dipolar groups, local and macroscopic effects, including interactions with Cs cations are explored.
Ralph Freund +6 more
wiley +1 more source
Zeeman Doppler Imaging of τ Ceti: The Weakest Magnetic Field Detected in a Sun-like Star
For nearly a decade, observations have shown that many older Sun-like stars spin faster than predicted, a phenomenon known as weakened magnetic braking (WMB). The leading hypothesis for WMB is a weakening of the large-scale dipole field, which leads to a
Federica Chiti +3 more
doaj +1 more source

