Cool Star Winds is a theoretical construct in astrophysics that models the persistent outflow of plasma and particles from the atmospheres of low-temperature stars, distinguished by its reliance on magnetic and wave-driven mechanisms rather than radiation pressure to drive mass loss.
104
Publications
6.3K
Citations
216
Authors
124
Institutions
Publications per year
2017–2026
16
Parents
Publications
104
Mechanisms for mass loss from cool stars
M. Morris · Publications of the Astronomical Society of the Pacific · 1987 · 239 citations · Full text
Natural Sciences, Astronomy, Physics +14
1–5 of 104
Authors
216
- DJ
6
h-index
- LHLee Hartmann
Center for Astrophysics Harvard & Smithsonian, United States
5 publications · 497 citations
5
h-index
- JH
4
h-index
- WH
4
h-index
- LD
4
h-index
1–5 of 216
Institutions
124
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
9 h-index
15 publications
1.5K citations
Goddard Space Flight Center
Greenbelt, United States
5 h-index
10 publications
251 citations
University of Potsdam
Potsdam, Germany
5 h-index
9 publications
502 citations
KU Leuven
Leuven, Belgium
4 h-index
16 publications
414 citations
University of Delaware
Newark, United States
4 h-index
5 publications
116 citations
Technische Universität Berlin
Berlin, Germany
4 h-index
7 publications
667 citations
University of America
Murrieta, United States
3 h-index
4 publications
127 citations
Australian National University
Canberra, Australia
3 h-index
5 publications
110 citations
1–8 of 124
Venues
- The Astrophysical Journal
ApJ · 46 publications · 3.3K citations
28
h-index
- Monthly Notices of the Royal Astronomical Society
16 publications · 712 citations
15
h-index
- Astronomy and Astrophysics
10 publications · 658 citations
10
h-index
- arXiv (Cornell University)
Repository · 2 publications · 33 citations
2
h-index
- AIPC
1 publications · 11 citations
1
h-index
1–5