Nebular Electron Density
Nebular Electron Density is a physical quantity in astrophysics that denotes the number of free electrons per unit volume within an ionized gas region, typically measured in electrons per cubic centimeter, and serves as a critical parameter for characterizing the ionization state and thermal structure of nebular environments.
283
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14.3K
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582
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256
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Publications per year
2017–2026
11
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283
Condensation in the primitive solar nebula
Lawrence Grossman · Geochimica et Cosmochimica Acta · 1972 · 1.1K citations
Natural Sciences, Astronomy, Physics +10
Astrophysics of gaseous nebulae
Donald E. Osterbrock · 1974 · 791 citations
Natural Sciences, Astronomy, Physics +12
Accumulation processes in the primitive solar nebula
A. G. W. Cameron · Icarus · 1973 · 278 citations
1–5 of 283
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University of California, Santa Cruz, United States
9 publications · 1.4K citations
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7
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7
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256
Instituto de Astrofísica de Canarias
Tenerife, Spain
16 h-index
32 publications
2.5K citations
University College London
London, United Kingdom
16 h-index
29 publications
1.8K citations
Universidad Nacional Autónoma de México
Mexico City, Mexico
11 h-index
22 publications
1.6K citations
Goddard Space Flight Center
Greenbelt, United States
10 h-index
19 publications
923 citations
National Radio Astronomy Observatory
Charlottesville, United States
9 h-index
12 publications
616 citations

Space Telescope Science Institute
Baltimore, United States
9 h-index
11 publications
790 citations
Instituto de Astrofísica de Andalucía
Granada, Spain
8 h-index
17 publications
434 citations

Peking University
Beijing, China
7 h-index
16 publications
1K citations
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ApJ · 92 publications · 3.8K citations
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48 publications · 2.2K citations
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25 publications · 868 citations
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PASP · 12 publications · 737 citations
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AJ · 13 publications · 445 citations
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