Dynamical Heating is a stellar dynamical process in which the velocity dispersion of stars in a galactic disk gradually increases over time due to gravitational interactions with transient structures such as spiral arms, molecular clouds, or satellite galaxies.
119
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8K
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389
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251
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2017–2026
39
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Publications
119
Simulations of Early Structure Formation: Primordial Gas Clouds
Naoki Yoshida, Tom Abel, Lars Hernquist et al. · The Astrophysical Journal · 2003 · 569 citations · Full text
Natural Sciences, Astronomy, Physics +17
1–5 of 119
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389
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3
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3
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3
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1–5 of 389
Institutions
251
University of Washington
Seattle, United States
8 h-index
20 publications
3.6K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
7 h-index
11 publications
2.5K citations
Centre National de la Recherche Scientifique
Paris, France
6 h-index
18 publications
452 citations
Space Telescope Science Institute
Baltimore, United States
6 h-index
9 publications
957 citations
Institute of Astronomy
Moscow, Russia
5 h-index
9 publications
1K citations
University of Hawaiʻi at Mānoa
Honolulu, United States
5 h-index
12 publications
638 citations
Goddard Space Flight Center
Greenbelt, United States
5 h-index
16 publications
1.3K citations
University College London
London, United Kingdom
5 h-index
10 publications
741 citations
1–8 of 251
Venues
- Monthly Notices of the Royal Astronomical Society
27 publications · 2.1K citations
20
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- The Astrophysical Journal
ApJ · 21 publications · 1.9K citations
18
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- Geophysical Research Letters
10 publications · 386 citations
10
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- Journal of Geophysical Research Atmospheres
JGR · 8 publications · 479 citations
8
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- Journal of Climate
5 publications · 237 citations
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