Nebular Abundances is a scientific construct in astrophysics that refers to the measured relative quantities of chemical elements in ionized interstellar gas regions, particularly H II regions, derived from emission line spectroscopy to characterize the elemental composition distinct from stellar abundances.
996
Publications
57.5K
Citations
1.8K
Authors
641
Institutions
Publications per year
2017–2026
88
Publications
996
PyNeb: a new tool for analyzing emission lines
V. Luridiana, C. Morisset, Richard A. Shaw · Astronomy and Astrophysics · 2014 · 647 citations · Full text
Natural Sciences, Astronomy, Physics +14
1–5 of 996
Authors
1.8K
- MJ
21
h-index
- LH
21
h-index
- MP
20
h-index
- CE
19
h-index
- JG
18
h-index
1–5 of 1.8K
Institutions
641
Centre National de la Recherche Scientifique
Paris, France
39 h-index
135 publications
10.3K citations
University College London
London, United Kingdom
36 h-index
100 publications
8K citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
32 h-index
139 publications
7.7K citations
Universidad Nacional Autónoma de México
Mexico City, Mexico
30 h-index
100 publications
6.3K citations
University of California, Los Angeles
Los Angeles, United States
28 h-index
68 publications
3.6K citations
University of Arizona
Tucson, United States
26 h-index
62 publications
4.2K citations
Goddard Space Flight Center
Greenbelt, United States
25 h-index
52 publications
2.4K citations
Universidad de La Laguna
San Cristóbal de La Laguna, Spain
25 h-index
81 publications
4.1K citations
1–8 of 641
Venues
- The Astrophysical Journal
ApJ · 335 publications · 19.5K citations
74
h-index
- Monthly Notices of the Royal Astronomical Society
167 publications · 11.7K citations
58
h-index
- Astronomy and Astrophysics
113 publications · 6.7K citations
49
h-index
- The Astrophysical Journal Supplement Series
26 publications · 2.7K citations
24
h-index
- Geochimica et Cosmochimica Acta
22 publications · 2K citations
21
h-index
1–5