Results 221 to 230 of about 89,722 (300)
Augmenting astrophysical scaling relations with machine learning: Application to reducing the Sunyaev-Zeldovich flux-mass scatter. [PDF]
Wadekar D+9 more
europepmc +1 more source
Abstract We investigate the melt production of planetary impacts as a function of planet size (R/REarth $R/{R}_{\text{Earth}}$ = 0.1–1.5), impactor size (L $L$ = 1–1,000 km), and core size ratio (Rcore/R ${R}_{\text{core}}/R$ = 0.2–0.8) using a combination of parameterized convection models and fully dynamical 2D impact simulations.
Lukas Manske+6 more
wiley +1 more source
Strongly lensed supernovae: lessons learned. [PDF]
Goobar A+2 more
europepmc +1 more source
Abstract How much of Io's SO2 ${\text{SO}}_{2}$ atmosphere is driven by volcanic outgassing or sublimation of SO2 ${\text{SO}}_{2}$ surface frost is a question with a considerable history. We develop a time dependent surface temperature model including thermal inertia and the exact celestial geometry to model the radiation driven global structure and ...
A.‐C. Dott+5 more
wiley +1 more source
Unveiling the evolution of rotating black holes in loop quantum cosmology. [PDF]
Swain S, Sahoo G, Nayak B.
europepmc +1 more source
Frequency-based redshift for cosmological observation and Hubble diagram from the 4-D spherical model in comparison with observed supernovae [PDF]
Shigeto Nagao
openalex +1 more source
Solar Wind‐Magnetosphere Coupling Under Interim Steady Conditions
Abstract Solar wind—magnetosphere coupling is an important driver of dynamics within the magnetosphere–ionosphere–thermosphere system, traditionally modeled using coupling functions. Most coupling functions assume the interaction is one‐directional, that the solar wind conditions determine the energy that is transferred into the magnetosphere.
A. Brenner+2 more
wiley +1 more source
Cosmic mysteries and the hydrogen 21-cm line: bridging the gap with lunar observations. [PDF]
Fialkov A, Gessey-Jones T, Dhandha J.
europepmc +1 more source
Predictions for the Shape and Orientation of Earth's Foreshock Radiation Sources
Abstract Radio emission produced in Earth's foreshock is due to the bow shock reflecting some electrons back upstream into the foreshock, where they produce Langmuir waves and radio emissions near the electron plasma frequency fp ${f}_{p}$ and near 2fp $2{f}_{p}$.
Iver H. Cairns, Patrick Oppel
wiley +1 more source