Yang Chen
Astronomy and Astrophysics · with Bressan · 2014–2019
A researcher in the Science corpus: 4 papers; trusts 7 researchers and is trusted by 6 researchers here, as inferred from the citation graph.
Subfields
- Astronomy and Astrophysics — 134 citations into it; #4,717 of 10,964 by trust here, #5,779 by citations
- Instrumentation — 78 citations into it; #1,425 of 3,502 by trust here, #2,432 by citations
Whom Yang Chen trusts overall
Their strongest outbound trust, strongest first, inferred from their citations.
- L. Girardi
- P. Marigo
- A. Bressan
- W. Hamann
- Martin Asplund
- Bernd Freytag
- G. Graefener
- G. Bertelli
- G. Gräfener
- E. Caffau
Who trusts Yang Chen overall
- Michela Mapelli
- N. Giacobbo
- Mario Spera
- John J. Vickers
- Martin C. Smith
- V. Belokurov
- A. Bressan
- M. Pecaut
- Julia Gutkin
- A. Mann
Papers from Yang Chen's perspective
Ordered by how strongly the researchers Yang Chen trusts endorse each paper. Same corpus, a different order for every researcher.
- The chemical composition of the Sun
- The Two Micron All Sky Survey (2MASS)
- On the variation of the initial mass function
- Solar Chemical Abundances Determined with a CO5BOLD 3D Model Atmosphere
- Theoretical isochrones in several photometric systems I. Johnson-Cousins-Glass, HST/WFPC2, HST/NICMOS, Washington, and ESO Imaging Survey filter sets
- WINDS FROM HOT STARS
- The empirical metallicity dependence of the mass-loss rate of O- and early B-type stars
- Mass loss from late-type WN stars and its Z-dependence: very massive stars approaching the Eddington limit
- Grids of stellar models with rotation - I. Models from 0.8 to 120 M⊙ at solar metallicity (Z = 0.014)
- Physical Properties of Wolf-Rayet Stars
Their papers
- Constraining the thermally pulsing asymptotic giant branch phase with resolved stellar populations in the Large Magellanic Cloud (2019) — 146 citations
- A NEW GENERATION OF PARSEC-COLIBRI STELLAR ISOCHRONES INCLUDING THE TP-AGB PHASE (2017) — 682 citations
- PARSEC evolutionary tracks of massive stars up to 350 M ☉ at metallicities 0.0001 ≤ Z ≤ 0.04 (2015) — 399 citations
- Improving PARSEC models for very low mass stars (2014) — 465 citations