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Stellar magnetic field
Rotation Period and Magnetic Field Morphology of the White Dwarf WD
Sun – Part 19 – Magnetic Field 1
Origin of Magnetic Fields in Cataclysmic Variables
Chandra X-Ray Study Confirms That the Magnetic Standard Ap Star KQ Vel
Radio Emission from Exoplanets: the Role of the Stellar Coronal Density and Magnetic Field Strength
Testing the Fossil Field Hypothesis: Could Strongly Magnetised OB Stars Produce All Known Magnetars?
Radio and High-Energy Emission of Pulsars Revealed by General Relativity Q
Arxiv:2002.08727V1 [Astro-Ph.EP] 20 Feb 2020
Spectropolarimetry
Dynamos and Magnetic Fields of the Sun and Other Cool Stars, and Their Role in the Formation and Evolution of Stars and in the Habitability of Planets
Magnetic Field on Brown Dwarf LSR J18353790+3259545
Magnetic Deformation of the White Dwarf Surface Structure
Torque Enhancement, Spin Equilibrium, and Jet Power From
Garraffo 2017 Apjl 843 L33.Pdf
Magnetic Fields from Very Low Mass Stars to Brown Dwarfs
Universe of Binaries, Binaries in the Universe
Magnetic Fields from Low-Mass Stars to Brown Dwarfs Julien Morin
197 9Apj. . .232 . .259G the Astrophysical Journal
Top View
Arxiv:1605.04979V1 [Astro-Ph.SR] 16 May 2016 2 M
Simulating Radio Emission from Low-Mass Stars
Measuring Stellar Magnetic Fields from High Resolution Spectroscopy Of
Impacts of Stellar Evolution and Dynamics on the Habitable Zone: the Role of Rotation and Magnetic Activity F
Gregg Hallinan National Radio Astronomy Observatory
Many Aspects of Magnetic Fields in Neutron Stars
Kilohertz Quasi-Periodic Oscillations, Magnetic Fields and Mass of Neutron Stars in Low-Mass X-Ray Binaries
Measurements of Stellar Magnetic Fields Using Synthetic Spectrum Fitting
Observations of Magnetic Fields on Late-Type Stars and Brown Dwarfs
The Impact of the SKA on Galactic Radioastronomy: Continuum
E-ELT Spectropolarimetry: the Science Case
Iaus331 Postmeetingreport V3.Pdf
1709.02861.Pdf
Angular Momentum Transfer in Star-Disk Interaction with Complex Stellar Magnetic Field M
Shape and Evolution of Wind-Blown Bubbles of Massive Stars: on the Effect of the Interstellar Magnetic field A
Stellar Physics with High-Resolution Uv
Accretion and Current Discs Controlled by Strong Magnetic Field
Pos(FRAPWS2016)045 fields field Dissipation field of Radio Pulsars
The Magnetic Field of the Planet Hosting Young Star Ci Tau
Arxiv:1612.03388V1 [Astro-Ph.SR] 11 Dec 2016 Possible Impact of the Solar Variability on the Terrestrial Cli- Magnetic fields in Cool Stars
Upgrading the Solar-Stellar Connection: News About Activity in Cool Stars
A Novel Look at the Pulsar Force-Free Magnetosphere 3
Magnetic Field Evolution During Neutron Star Recycling
An Overview of Stellar Radio Astronomy
Magnetic Field in Neutron Stars
Neutron Star Electromagnetic Field Structure Hugh O
A Clue to the Origin of Neutron Star Magnetic Fields? V
Gravitational Waves from Single Neutron Stars: an Advanced Detector Era Survey
Features of the Accretion in the EX Hydrae System
Arxiv:2105.03387V1 [Astro-Ph.SR] 7 May 2021 Have Surface Magnetic fields of B = 107 G Or Larger And, in Ref
Activity and Magnetic Field Structure of the Sun-Like Planet-Hosting Star HD
A Universal Relation for the Propeller Mechanisms in Magnetic Rotating
Stellar Physics with High-Resolution UV Spectropolarimetry
On the Precession of the Isolated Pulsar PSR B1828-11
Disk Accretion Onto a Magnetized Star
Modelling Exoplanetary Radio Emissions Using a Realistic Magnetic Field Geometry
Techniques for Stellar Magnetic Field Measurements
Evidence of Magnetic Field Decay in Massive Main-Sequence Stars
The Formation and Early Evolution of Low-Mass Stars and Brown Dwarfs
Simulating Radio Emission from Low-Mass Stars
The Magnetic Sun CESAR’S Booklet
Observations of Cool-Star Magnetic Fields
Flare Stars: a Short Review Krstinja Dzombeta Department of Astronomy and Astrophysics, University of Toronto Toronto on Canada
Numerical Modelling of Astrospheres
Observing Stellar Magnetic Fields & Activity Magnetic Fields & Activity
Modeling Magnetohydrodynamic Equilibrium in Magnetars with Applications to Continuous Gravitational Wave Production
Pulsating Stars--Plethora of Variables and Observational Tasks