A. Maeder
Impact in
- Instrumentation top 10%
- Astronomy and Astrophysical Research
- Astronomy and Astrophysics top 10%
- Stellar, planetary, and galactic studies
- Astrophysics and Star Formation Studies
- Gamma-ray bursts and supernovae
- Astro and Planetary Science
- Galaxies: Formation, Evolution, Phenomena
- Pulsars and Gravitational Waves Research
- Astrophysical Phenomena and Observations
Papers in
-
- Stellar, planetary, and galactic studies 17
- Galaxies: Formation, Evolution, Phenomena 3
- Astrophysics and Star Formation Studies 2
- History and Developments in Astronomy 2
- Solar and Space Plasma Dynamics 2
-
- Astronomy and Astrophysical Research 17
- Co-authors
- G. Meynet (5 shared papers)N. Langer (1 shared paper)Stanford E. Woosley (1 shared paper)J. Audouze (1 shared paper)B. Hauck (1 shared paper)C. Chiosi (1 shared paper)B. Barbuy (1 shared paper)J. R. De Medeiros (1 shared paper)
- Journals
- Astronomy and Astrophysics (1 paper)A&A (2 papers)arXiv (Cornell University) (1 paper)CERN Document Server (European Organization for Nuclear Research) (1 paper)The Messenger (1 paper)
- Partner nations
- Switzerland
In The Last Decade
A. Maeder
18 papers receiving 112 citations
Peers
Comparison fields: 5 of 16
- Instrumentation 37
- Astronomy and Astrophysics 121
- Nuclear and High Energy Physics 14
- Geophysics 5
- Computational Mechanics 6
Countries citing papers authored by A. Maeder
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
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-authors
The 22 scholars most cited alongside A. Maeder, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.
All Works
Showing the 20 most-cited of 23 papers — load more, or switch the sort, to bring in the rest.
| # | Work | ||
|---|---|---|---|
| 1 | Stellar yields as a function of initial metallicity and mass limit for black hole formation | 1992 | 25 |
| 2 | Nucleosynthesis and chemical evolution : sixteenth advanced course of the Swiss Society of Astronomy and Astrophysics | 1986 | 21 |
| 3 | Tables of evolutionary star modles from 0.85 to 120 solar mass with overshooting and mass loss. | 1988 | 15 |
| 4 | The most massive stars evolving to red supergiants - Evolution with mass loss, WR stars as post-red supergiants and pre-supernovae | 1981 | 12 |
| 5 | The problem of the blue-to-red supergiant ratio in galaxies. | 1995 | 9 |
| 6 | The most massive stars in the Galaxy and the LMC - Quasi-homogeneous evolution, time-averaged mass loss rates and mass limits | 1980 | 8 |
| 7 | Four basic solar and stellar tests of cosmologies with variable past G and macroscopic masses. | 1977 | 7 |
| 8 | Luminosity and T eff determinations for B-type stars. | 1979 | 6 |
| 9 | Catalogue of photometric data related to surface magnetic fields for B-type stars. | 1980 | 5 |
| 10 | ABOUT THE ABSENCE OF A PROPER ZERO AGE MAIN SEQUENCE FOR MASSIVE STARS | 1996 | 4 |
| 11 | Relation between surface magnetic field intensities and Geneva photometry | 1980 | 3 |
| 12 | Topical astrophysical problems on massive stars for VLT observations. | 1995 | 2 |
| 13 | Carbon, nitrogen and oxygen abundances in yellow supergiants. | 1996 | 2 |
| 14 | Observational tests on star formation. II. Variation of the axial rotational velocities with the galacto-centric distance, for early B-type stars in the local spiral arm. | 1977 | 1 |
| 15 | Photometric classification of B and AP stars with an application to 3600 stars | 1981 | 1 |
| 16 | 1997 | 1 | |
| 17 | 1995 | 1 | |
| 18 | Evidences for a bifurcation in massive star evolution. | 1986 | 1 |
| 19 | The number of Wolf-Rayet stars in Local Group galaxies. | 1988 | 0 |
| 20 | Nucleosynthesis in massive stars | 2000 | 0 |
About A. Maeder
A. Maeder is a scholar working on Astronomy and Astrophysics, Instrumentation, Computational Mechanics, Mechanical Engineering and Applied Mathematics, having authored 23 papers that have together received 124 indexed citations. Recurring topics across this work include Stellar, planetary, and galactic studies (17 papers), Astronomy and Astrophysical Research (17 papers), Astronomical Observations and Instrumentation (7 papers), Galaxies: Formation, Evolution, Phenomena (3 papers), Astrophysics and Star Formation Studies (2 papers), History and Developments in Astronomy (2 papers), Solar and Space Plasma Dynamics (2 papers) and Material Science and Thermodynamics (1 paper). The work is most often cited by research in Instrumentation (37 citations), Astronomy and Astrophysics (121 citations), Nuclear and High Energy Physics (14 citations), Geophysics (5 citations) and Computational Mechanics (6 citations). A. Maeder has collaborated with scholars based in Switzerland. Frequent co-authors include G. Meynet, N. Langer, Stanford E. Woosley, J. Audouze, B. Hauck, C. Chiosi, B. Barbuy, J. R. De Medeiros, G. Burki and D. Schaerer. Their work appears in journals such as Astronomy and Astrophysics, A&A, arXiv (Cornell University), CERN Document Server (European Organization for Nuclear Research) and The Messenger.
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.