Nebular Electron Temperature is the characteristic thermal energy of free electrons in an ionized nebular gas, typically measured through the ratio of emission lines sensitive to electron collisions, distinguishing it from other gas temperature indicators by its direct dependence on electron impact excitation processes.
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221
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Publications per year
2017–2026
12
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Publications
204
1–5 of 204
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413
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11
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11
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10
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8
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7
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1–5 of 413
Institutions
221
University College London
London, United Kingdom
17 h-index
45 publications
3.2K citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
11 h-index
21 publications
1.3K citations
Peking University
Beijing, China
10 h-index
23 publications
1.4K citations
Goddard Space Flight Center
Greenbelt, United States
9 h-index
22 publications
592 citations
Universidad Nacional Autónoma de México
Mexico City, Mexico
9 h-index
18 publications
1.4K citations
Australian National University
Canberra, Australia
8 h-index
17 publications
859 citations
University of Kentucky
Lexington, United States
8 h-index
9 publications
236 citations
National Radio Astronomy Observatory
Charlottesville, United States
7 h-index
9 publications
457 citations
1–8 of 221
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- Monthly Notices of the Royal Astronomical Society
55 publications · 3K citations
31
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- The Astrophysical Journal
ApJ · 60 publications · 2.6K citations
26
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- Astronomy and Astrophysics
22 publications · 779 citations
16
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- Publications of the Astronomical Society of the Pacific
PASP · 11 publications · 822 citations
11
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- The Astronomical Journal
AJ · 9 publications · 635 citations
9
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