A. Maeder

17.6k total citations · 2 hit papers
240 papers, 10.8k citations indexed

About

A. Maeder is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, A. Maeder has authored 240 papers receiving a total of 10.8k indexed citations (citations by other indexed papers that have themselves been cited), including 233 papers in Astronomy and Astrophysics, 106 papers in Instrumentation and 15 papers in Nuclear and High Energy Physics. Recurrent topics in A. Maeder's work include Stellar, planetary, and galactic studies (199 papers), Astro and Planetary Science (107 papers) and Astronomy and Astrophysical Research (106 papers). A. Maeder is often cited by papers focused on Stellar, planetary, and galactic studies (199 papers), Astro and Planetary Science (107 papers) and Astronomy and Astrophysical Research (106 papers). A. Maeder collaborates with scholars based in Switzerland, United Kingdom and France. A. Maeder's co-authors include G. Meynet, Raphaël Hirschi, Sylvia Ekström, P. Eggenberger, C. Georgy, C. Charbonnel, A. Granada, N. Mowlavï, T. Decressin and U. Frischknecht and has published in prestigious journals such as Nature, Reviews of Modern Physics and The Astrophysical Journal.

In The Last Decade

A. Maeder

219 papers receiving 10.3k citations

Hit Papers

Grids of stellar models with rotation 2011 2026 2016 2021 2011 2012 250 500 750 1000

Peers

A. Maeder
Comparison fields: 5 of 92
  • Astronomy and Astrophysics 10.4k
  • Instrumentation 3.4k
  • Nuclear and High Energy Physics 949
  • Computational Mechanics 249
  • Atomic and Molecular Physics, and Optics 137
Replace G. Meynet with:
G. Meynet Switzerland
Marc H. Pinsonneault United States
C. Mordasini Switzerland
J. Andersen United States
C. A. Pilachowski United States
P. Demarque United States
P. François France
William E. Harris Canada
Raphaël Hirschi United Kingdom
H.‐G. Ludwig Germany
G. Meynet Switzerland View profile →
Citations per field, relative to A. Maeder
A. Maeder · 1×
Citations per year, relative to A. Maeder
A. Maeder · 1×

Countries citing papers authored by A. Maeder

Since Specialization
Citations

This map shows the geographic impact of A. Maeder's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by A. Maeder with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites A. Maeder more than expected).

Fields of papers citing papers by A. Maeder

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by A. Maeder. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by A. Maeder. The network helps show where A. Maeder may publish in the future.

Co-authorship network of co-authors of A. Maeder

This figure shows the co-authorship network connecting the top 25 collaborators of A. Maeder. A scholar is included among the top collaborators of A. Maeder based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with A. Maeder. A. Maeder is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

20 of 20 papers shown
# Work Indexed citations
1 4
2 7
3 34
4
What helium and lithium can tell us about CEMP stars?
0
5 23
6 52
7 20
8 35
9
Grids of stellar models with rotation : I. Models from 0.8 to 120 M⊙ at solar metallicity (Z = 0.014) breakdown →
684
10 105
11 36
12 69
13 185
14 35
15
The Conti scenario for forming WR stars: past, present and future
0
16
New models of Wolf-Rayet stars and comparison with data in galaxies
4
17
Grids of massive stars with high mass loss rates. V. From 12 to 120 M sun _ at Z=0.001, 0.004, 0.008, 0.020 and 0.040
18
18
New dating of galactic open clusters.
9
19
Grids of evolutionary models of massive stars with mass loss and overshooting - Properties of Wolf-Rayet stars sensitive to overshooting.
24
20
Supergiant variability: theoretical pulsation periods and comparison with observations
3

Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.

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