Stellar Luminosity Evolution
Stellar Luminosity Evolution is the time-dependent change in a star's total electromagnetic energy output per unit time, distinguishing it from static luminosity measures by characterizing how stellar brightness varies across its evolutionary phases due to internal structural and compositional changes.
286
Publications
29.9K
Citations
1.1K
Authors
389
Institutions
Publications per year
2017–2026
33
286
Charlie Conroy, James E. Gunn, Martin White · The Astrophysical Journal · 2009 · 1.9K citations · Full text
Natural Sciences, Astronomy, Physics +17
1–5 of 286
1.1K
4
h-index
4
h-index
4
h-index
3
h-index
3
h-index
1–5 of 1.1K
389
California Institute of Technology
Pasadena, United States
17 h-index
50 publications
5.6K citations

Centre National de la Recherche Scientifique
Paris, France
12 h-index
43 publications
3.9K citations
Institute of Astronomy
Moscow, Russia
11 h-index
24 publications
9.7K citations
University of California, Berkeley
Berkeley, United States
11 h-index
28 publications
5.3K citations
University of Cambridge
Cambridge, United Kingdom
11 h-index
20 publications
1.5K citations
University of California, Santa Cruz
Santa Cruz, United States
10 h-index
31 publications
3.9K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
10 h-index
18 publications
1.1K citations
Leiden University
Leiden, The Netherlands
10 h-index
22 publications
4.7K citations
1–8 of 389
ApJ · 146 publications · 14.1K citations
59
h-index
46 publications · 6.9K citations
29
h-index
22 publications · 1.4K citations
17
h-index
AJ · 12 publications · 682 citations
11
h-index
10 publications · 2.6K citations
10
h-index
1–5