Stephen R. Kane et al 2020 AJ 160 81
Dynamical models suggest that the width of the habitable zone for earlier-type stars allows for more terrestrial planets in the habitable zone than around late-type stars.
Ran Si et al 2020 ApJL 898 L34
A new methodology, based on a careful study of magnetic induced atomic transitions, is used to provide the first estimates of the coronal magnetic field strength using spectroscopic data from Hinode.
Rajani D. Dhingra et al 2020 Planet. Sci. J. 1 31
Analysis of bright ephemeral features on Titan’s north pole suggest that they represent either broad specular reflection off of a recently wetted surface or a near-surface fog — both owing to probable recent rainfalls.
Błażej Nikiel-Wroczyński et al 2020 ApJ 898 110
Radio polarimetric imaging indicates a magnetic structure within the Stephan’s Quintet galaxy system spanning at least 60 × 40 × 20 kpc, with a strength at least as high as that previously detected within large spiral galaxies.
Nau Raj Pokhrel et al 2020 AJ 160 66
A new catalog presents 306 holes identified in the neutral atomic hydrogen of 41 gas-rich dwarf galaxies in LITTLE THINGS, likely generated during the process of star formation.
Rebecca G. Martin et al 2020 ApJL 898 L26
Hydrodynamic modeling of tilt instabilities in accretion disks around binary systems shows that detached circumplanetary disks may commonly be misaligned relative to the planetary orbital plane.