Results 11 to 20 of about 5,710 (349)
The energy budget of stellar magnetic fields [PDF]
VS acknowledges the support of an Science & Technology Facilities Council (STFC) studentship. AAV acknowledges support from the Swiss National Science Foundation through an Ambizione Fellowship.
M Jardine, A A Vidotto, J -F Donati
exaly +9 more sources
Stellar evolution with rotation and magnetic fields [PDF]
We compare the current effects of rotation in stellar evolution to those of the magnetic field created by the Tayler instability. In stellar regions, where a magnetic field can be generated by the dynamo due to differential rotation (Spruit [CITE ...
A Maeder
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Magnetic fields and stellar oscillations
Stars are fluid bodies in which pressure, buoyancy, rotation and magnetism provide the restoring forces for wave propagation. Constructive interference of these waves generates global modes of oscillation.
Shyeh Tjing Loi
core +5 more sources
Evolution of Stellar Magnetic Fields [PDF]
AbstractStellar magnetic fields can reliably be characterized by several magnetic activity indicators, such as X-ray or radio luminosity. Physical processes leading to such emission provide important information on dynamic processes in stellar atmospheres and magnetic structuring.
M. Güdel
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Mapping Stellar Magnetic Fields [PDF]
12 pages, 2 figures; conference proceedings "Stellar Magnetic Fields - A workshop in honour of the career and contributions of John Landstreet", London, Canada ...
O. Kochukhov
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Magnetic Fields and Stellar Evolution [PDF]
Magnetic fields are now observed or inferred in a wide variety of stellar objects. The class of early-type stars with strong large-scale fields extends from types B to F, with effective fields from 300 gauss up to several x 104 gauss (Borra and Landstreet 1980).
L. Mestel
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Measuring the magnetic fields in the chromospheres of low-mass stars [PDF]
Magnetic fields in the upper atmospheres of solar-like stars are believed to provide an enormous amount of energy to power the hot coronae and drive large-scale eruptions that could impact the habitability of planetary systems around these stars. However,
Tianqi Cang +13 more
doaj +3 more sources
The magnetic fields and stellar winds of the mature late F-stars: β Virginis and θ Draconis [PDF]
International audienceMapping the large-scale magnetic field in late F-type stars is important for understanding the nature of the stellar dynamo and the dynamics of thin outer convection zones.
J. Seach +6 more
openalex +3 more sources
Impact of non-uniform surface magnetic fields on stellar winds [PDF]
Observations of active stars reveal highly non-uniform surface distributions of magnetic flux. Theoretical models considering magnetised stellar winds however often presume uniform surface magnetic fields, characterised by a single magnetic field ...
V. Holzwarth
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Stable magnetic fields in stellar interiors [PDF]
19 pages, 24 figures, submitted to A& ...
J Braithwaite, Åke Nordlund
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