Magnetically Driven Stellar Winds
Magnetically Driven Stellar Winds is a theoretical model of stellar mass loss in which the acceleration and structuring of outflowing plasma are predominantly governed by magnetic fields originating from the stellar interior, distinguishing it from thermally or radiatively driven wind mechanisms.
248
Publications
19.5K
Citations
505
Authors
337
Institutions
Publications per year
2017–2026
54
Parents
248
Shapes and Shaping of Planetary Nebulae
Bruce Balick, Adam Frank · Annual Review of Astronomy and Astrophysics · 2002 · 638 citations
Natural Sciences, Astronomy, Physics +10
Angular momentum loss in low-mass stars
S. D. Kawaler · The Astrophysical Journal · 1988 · 596 citations
Natural Sciences, Astronomy, Physics +16
Magnetic Braking by a Stellar Wind--I
L. Mestel · Monthly Notices of the Royal Astronomical Society · 1968 · 558 citations · Full text
Natural Sciences, Astronomy, Physics +16
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505
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337

Centre National de la Recherche Scientifique
Paris, France
18 h-index
42 publications
2.2K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
17 h-index
28 publications
2.1K citations
University of Delaware
Newark, United States
11 h-index
21 publications
2K citations
The University of Tokyo
Tokyo, Japan
11 h-index
18 publications
709 citations
University of California, Berkeley
Berkeley, United States
11 h-index
18 publications
2K citations
University of Wisconsin–Madison
Madison, United States
8 h-index
22 publications
725 citations

University of St Andrews
St Andrews, United Kingdom
8 h-index
16 publications
1.4K citations
Université Paris Cité
Paris, France
8 h-index
13 publications
652 citations
1–8 of 337
ApJ · 103 publications · 9.4K citations
49
h-index
65 publications · 4.1K citations
36
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16 publications · 672 citations
15
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8 publications · 609 citations
8
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AJ · 6 publications · 249 citations
6
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