Open Cluster Spectroscopy
Open Cluster Spectroscopy is a spectroscopic method that systematically analyzes the collective spectral characteristics of stars within open clusters to determine their physical properties, chemical compositions, and evolutionary states, distinguishing it from broader stellar spectroscopy by its focused application to coeval, gravitationally unbound stellar populations.
441
Publications
21.8K
Citations
1.1K
Authors
445
Institutions
Publications per year
2017–2026
79
Parents
441
The Old Open Clusters of the Milky Way
E. D. Friel · Annual Review of Astronomy and Astrophysics · 1995 · 482 citations
Natural Sciences, Astronomy, Physics +15
Metallicities of Old Open Clusters
Eileen D. Friel, K. A. Janes, M. Tavarez et al. · The Astronomical Journal · 2002 · 378 citations · Full text
1–5 of 441
1.1K
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445
Instituto de Astrofísica de Canarias
Tenerife, Spain
28 h-index
104 publications
7.3K citations
Osservatorio Astronomico di Padova
Padua, Italy
28 h-index
112 publications
7K citations
Arcetri Astrophysical Observatory
Florence, Italy
27 h-index
107 publications
7.4K citations
European Southern Observatory
Santiago, Chile
25 h-index
43 publications
2.7K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
24 h-index
51 publications
2.5K citations
Indiana University Bloomington
Bloomington, United States
23 h-index
48 publications
2.4K citations

Universidad de La Laguna
San Cristóbal de La Laguna, Spain
22 h-index
73 publications
4.4K citations

U.S. National Science Foundation
Alexandria, United States
21 h-index
39 publications
2.7K citations
1–8 of 445
120 publications · 5.9K citations
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AJ · 76 publications · 4.4K citations
38
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ApJ · 64 publications · 3.9K citations
32
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65 publications · 2.4K citations
27
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Repository · 16 publications · 546 citations
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