M. Limongi
Astronomy and Astrophysics · 2000–2018
A researcher in the Science corpus: 8 papers; trusts 54 researchers and is trusted by 74 researchers here, as inferred from the citation graph.
Subfields
- Astronomy and Astrophysics — 127 citations into it; #799 of 10,964 by trust here, #3,373 by citations
- Instrumentation — 51 citations into it
- Nuclear and High Energy Physics — 34 citations into it; #1,005 of 6,161 by trust here, #3,136 by citations
- Statistical and Nonlinear Physics — 8 citations into it
- Aerospace Engineering — 6 citations into it
- Computational Mechanics — 5 citations into it
Whom M. Limongi trusts overall
Their strongest outbound trust, strongest first, inferred from their citations.
- A. Chieffi
- G. Meynet
- Andre Maeder
- S. Smartt
- I. Hunter
- Sung-Chul Yoon
- Alexander Heger
- R. Hirschi
- I. Brott
- Martin Asplund
Who trusts M. Limongi overall
- A. Chieffi
- R. Hirschi
- Stan Woosley
- Krzysztof Belczyński
- Ken'ichi Nomoto
- Nozomu Tominaga
- C. Kobayashi
- E. O’Connor
- Maurizio Salaris
- G. Meynet
Papers from M. Limongi's perspective
Ordered by how strongly the researchers M. Limongi trusts endorse each paper. Same corpus, a different order for every researcher.
- The Progenitor Stars of Gamma-Ray Bursts
- The chemical composition of the Sun
- How Massive Single Stars End Their Life
- Grids of stellar models with rotation - I. Models from 0.8 to 120 M⊙ at solar metallicity (Z = 0.014)
- Stellar evolution with rotation. VII. - Low metallicity models and the blue to red supergiant ratio in the SMC
- Progenitors of Core-Collapse Supernovae
- First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy
- Stellar evolution with rotation XII. Pre-supernova models
- An Empirical formula for the mass-loss rates of dust-enshrouded red supergiants and oxygen-rich asymptotic giant branch stars
- Presupernova Evolution of Rotating Massive Stars. II. Evolution of the Surface Properties
Their papers
- Presupernova Evolution and Explosive Nucleosynthesis of Rotating Massive Stars in the Metallicity Range −3 ≤ [Fe/H] ≤ 0 (2018) — 323 citations
- Chemical evolution with rotating massive star yields - I. The solar neighbourhood and the s-process elements (2018) — 196 citations
- PRE-SUPERNOVA EVOLUTION OF ROTATING SOLAR METALLICITY STARS IN THE MASS RANGE 13–120 M☉ AND THEIR EXPLOSIVE YIELDS (2012) — 211 citations
- The Nucleosynthesis of 26Al and 60Fe in Solar Metallicity Stars Extending in Mass from 11 to 120 M☉: The Hydrostatic and Explosive Contributions (2006) — 329 citations
- Explosive Yields of Massive Stars from Z = 0 to Z = Z☉ (2004) — 290 citations
- Evolution, Explosion, and Nucleosynthesis of Core-Collapse Supernovae (2003) — 201 citations
- The White Dwarf Cooling Sequence of the Globular Cluster Messier 4 (2002) — 209 citations
- Massive Stars in the Range 13-25 M⊙: Evolution and Nucleosynthesis. II. The Solar Metallicity Models (2000) — 136 citations