Hydrodynamics of core-collapse supernovae and their progenitors

B Müller - Living Reviews in Computational Astrophysics, 2020‏ - Springer
Multi-dimensional fluid flow plays a paramount role in the explosions of massive stars as
core-collapse supernovae. In recent years, three-dimensional (3D) simulations of these …

Solar dynamo theory

P Charbonneau - Annual Review of Astronomy and …, 2014‏ - annualreviews.org
The Sun's magnetic field is the engine and energy source driving all phenomena collectively
defining solar activity, which in turn structures the whole heliosphere and significantly …

The sloan digital sky survey quasar catalog: Sixteenth data release

BW Lyke, AN Higley, JN McLane… - The Astrophysical …, 2020‏ - iopscience.iop.org
We present the final Sloan Digital Sky Survey IV (SDSS-IV) quasar catalog from Data
Release 16 of the extended Baryon Oscillation Spectroscopic Survey (eBOSS). This catalog …

Dynamo theories

F Rincon - Journal of Plasma Physics, 2019‏ - cambridge.org
These lecture notes are based on a tutorial given in 2017 at a plasma physics winter school
in Les Houches. Their aim is to provide a self-contained graduate-student level introduction …

The Solar Optical Telescope for the Hinode Mission: An Overview

S Tsuneta, K Ichimoto, Y Katsukawa, S Nagata… - Solar Physics, 2008‏ - Springer
Abstract The Solar Optical Telescope (SOT) aboard the Hinode satellite (formerly called
Solar-B) consists of the Optical Telescope Assembly (OTA) and the Focal Plane Package …

Colloquium: Unusual dynamics of convection in the Sun

J Schumacher, KR Sreenivasan - Reviews of Modern Physics, 2020‏ - APS
The Sun is our nearest star; it is also the most important star that determines life on Earth. A
large variety of phenomena observed on the Sun's surface, with potential impact on Earth, is …

[HTML][HTML] Observations of cool-star magnetic fields

A Reiners - Living Reviews in Solar Physics, 2012‏ - Springer
Cool stars like the Sun harbor convection zones capable of producing substantial surface
magnetic fields leading to stellar magnetic activity. The influence of stellar parameters like …

Chromospheric activity catalogue of 4454 cool stars-Questioning the active branch of stellar activity cycles

SB Saikia, CJ Marvin, SV Jeffers, A Reiners… - Astronomy & …, 2018‏ - aanda.org
Context. Chromospheric activity monitoring of a wide range of cool stars can provide
valuable information on stellar magnetic activity and its dependence on fundamental stellar …

The effect of stellar contamination on low-resolution transmission spectroscopy: needs identified by NASA's Exoplanet Exploration Program Study Analysis Group 21

BV Rackham, N Espinoza… - RAS Techniques …, 2023‏ - academic.oup.com
Abstract Study Analysis Group 21 (SAG21) of NASA's Exoplanet Exploration Program
Analysis Group was organized to study the effect of stellar contamination on space-based …

The standard flare model in three dimensions-I. Strong-to-weak shear transition in post-flare loops

G Aulanier, M Janvier, B Schmieder - Astronomy & Astrophysics, 2012‏ - aanda.org
Context. The standard CSHKP model for eruptive flares is two-dimensional. Yet
observational interpretations of photospheric currents in pre-eruptive sigmoids, shear in post …