J. Groh
Astronomy and Astrophysics · 2013–2018
A researcher in the Science corpus: 4 papers; trusts 13 researchers and is trusted by 1 researcher here, as inferred from the citation graph.
Subfields
- Astronomy and Astrophysics — 116 citations into it; #10,418 of 10,964 by trust here, #8,034 by citations
- Instrumentation — 49 citations into it; #3,263 of 3,502 by trust here, #3,063 by citations
Whom J. Groh trusts overall
Their strongest outbound trust, strongest first, inferred from their citations.
- W. Hamann
- N. Smith
- R. Kudritzki
- G. Graefener
- N. Langer
- Andre Maeder
- J. Holberg
- Emily M. Levesque
- G. Meynet
- S. Smartt
Who trusts J. Groh overall
Papers from J. Groh's perspective
Ordered by how strongly the researchers J. Groh trusts endorse each paper. Same corpus, a different order for every researcher.
- Progenitors of Core-Collapse Supernovae
- Physical Properties of Wolf-Rayet Stars
- Grids of stellar models with rotation - I. Models from 0.8 to 120 M⊙ at solar metallicity (Z = 0.014)
- WINDS FROM HOT STARS
- An Empirical formula for the mass-loss rates of dust-enshrouded red supergiants and oxygen-rich asymptotic giant branch stars
- The Galactic WN stars. Spectral analyses with line-blanketed model atmospheres versus stellar evolut
- How Massive Single Stars End Their Life
- The Progenitor Stars of Gamma-Ray Bursts
- The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 M⊙ stellar mass limit
- The Effect of Massive Binaries on Stellar Populations and Supernova Progenitors (Proceedings of the International Astronomical Union)
Their papers
- Spectral models for binary products: Unifying subdwarfs and Wolf-Rayet stars as a sequence of stripped-envelope stars (2018) — 134 citations
- Confined dense circumstellar material surrounding a regular type II supernova (2017) — 269 citations
- Fundamental properties of core-collapse Supernova and GRB progenitors: predicting the look of massive stars before death (2013) — 151 citations
- Grids of stellar models with rotation - III. Models from 0.8 to 120 Msun at a metallicity Z = 0.002 (2013) — 155 citations