Disk Heating
Disk Heating is a theoretical construct in galactic dynamics that describes the process by which stellar orbits in a galactic disk increase in random motion and vertical oscillation amplitudes over time due to gravitational interactions with spiral arms, molecular clouds, or mergers, leading to disk thickening.
205
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18.1K
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430
Authors
265
Institutions
Publications per year
2017–2026
30
205
Accretion Disks around Young Objects. I. The Detailed Vertical Structure
Paola D’Alessio, J. Cantó, Nuria Calvet et al. · The Astrophysical Journal · 1998 · 647 citations · Full text
Natural Sciences, Astronomy, Physics +17
Nonlinear Outcome of Gravitational Instability in Cooling, Gaseous Disks
2001 · 582 citations
Natural Sciences, Astronomy, Physics +17
Heating of galactic disks by mergers
Peter J. Quinn, Lars Hernquist, D. P. Fullagar · The Astrophysical Journal · 1993 · 562 citations
Natural Sciences, Astronomy, Physics +14
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265

Centre National de la Recherche Scientifique
Paris, France
15 h-index
41 publications
2K citations
University of Washington
Seattle, United States
12 h-index
22 publications
2.7K citations
Institute of Astronomy
Moscow, Russia
10 h-index
11 publications
933 citations

Space Telescope Science Institute
Baltimore, United States
9 h-index
12 publications
858 citations
Max Planck Institute for Astronomy
Heidelberg, Germany
9 h-index
16 publications
1.3K citations
University of Cambridge
Cambridge, United Kingdom
8 h-index
11 publications
535 citations

University of Rochester
Rochester, United States
7 h-index
10 publications
951 citations
University of California, Santa Cruz
Santa Cruz, United States
7 h-index
10 publications
1K citations
1–8 of 265
ApJ · 63 publications · 9K citations
42
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42 publications · 3.4K citations
31
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21 publications · 858 citations
17
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AJ · 7 publications · 440 citations
7
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Repository · 4 publications · 190 citations
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