EVN observations of 6.7 GHz methanol maser polarization in massive star-forming regions III. The flux-limited sample [PDF]
, 2015 Theoretical simulations and observations at different angular resolutions have shown that magnetic fields have a central role in massive star formation.
Bartkiewicz, A. +5 more
core +3 more sources
Seismological insights into solar and stellar magnetic activity cycles
EPJ Web of Conferences, 2017 The Sun’s magnetic activity cycle varies primarily on a time scale of approximately 11yrs from minimum to maximum and back again. It is well-known that the properties of the Sun’s acoustic oscillations are affected by the near-surface internal magnetic ...
Broomhall Anne-Marie
doaj +1 more source
Magnetic fields in massive spirals: The role of feedback and initial conditions [PDF]
, 2018 Magnetic fields play a very important role in the evolution of galaxies through their direct impact on star formation and stellar feedback-induced turbulence.
Ntormousi, Evangelia
core +2 more sources
Stellar magnetic activity and exoplanets
EPJ Web of Conferences, 2017 It has been proposed that magnetic activity could be enhanced due to interactions between close-in massive planets and their host stars. In this article, I present a brief overview of the connection between stellar magnetic activity and exoplanets ...
Vidotto A.A.
doaj +1 more source
Magnetic Braking Formulation for Sun-Like Stars: Dependence on Dipole Field Strength and Rotation Rate [PDF]
, 2012 We use two-dimensional axisymmetric magnetohydrodynamic simulations to compute steady-state solutions for solar-like stellar winds from rotating stars with dipolar magnetic fields.
Barnes +20 more
core +4 more sources
Rotation Measure Variations and Reversals of Repeating FRBs in Massive Binary Systems
The Astrophysical Journal, 2023 Recent observations discovered that some repeating fast radio bursts (FRBs) show complicated variations and reversals of Faraday rotation measures (RMs), indicating that the sources of these FRBs are embedded in a dynamically magnetized environment.
Z. Y. Zhao +3 more
doaj +1 more source
Ultraviolet spectropolarimetry: investigating stellar magnetic field diagnostics
Astrophysics and Space Science, 2022 Accepted for publication in Astrophysics and Space Science; updated to accepted version.
Folsom, C. P. +11 more
openaire +6 more sources
Search for magnetic fields in particle-accelerating colliding-wind binaries [PDF]
, 2014 Some colliding-wind massive binaries, called particle-accelerating colliding-wind binaries (PACWB), exhibit synchrotron radio emission, which is assumed to be generated by a stellar magnetic field.
De Becker, M. +4 more
core +3 more sources
Modelling stellar coronal magnetic fields [PDF]
Proceedings of the International Astronomical Union, 2010 AbstractOur understanding of the structure and dynamics of stellar coronae has changed dramatically with the availability of surface maps of both star spots and also magnetic field vectors. Magnetic field extrapolations from these surface maps reveal surprising coronal structures for stars whose masses and hence internal structures and dynamo modes may
Jardine, Moira +3 more
openaire +2 more sources
The contribution of starspots to coronal structure [PDF]
, 2010 Significant progress has been made recently in our understanding of the structure of stellar magnetic fields, thanks to advances in detection methods such as Zeeman-Doppler Imaging.
Arzoumanian, Doris +4 more
core +2 more sources