H. Sawai

Astronomy and Astrophysics · 2016

A researcher in the Science corpus: 1 paper; trusts 1 researcher and is trusted by 0 researchers here, as inferred from the citation graph.

Subfields

• Astronomy and Astrophysics — 15 citations into it
• Nuclear and High Energy Physics — 8 citations into it

Whom H. Sawai trusts overall

Their strongest outbound trust, strongest first, inferred from their citations.

1. Friedrich-Karl Thielemann
2. T. Rauscher
3. N. Nishimura
4. Satoshi Honda

Papers from H. Sawai's perspective

Ordered by how strongly the researchers H. Sawai trusts endorse each paper. Same corpus, a different order for every researcher.

1. On the astrophysical robustness of the neutron star merger r-process
2. MAGNETOROTATIONALLY DRIVEN SUPERNOVAE AS THE ORIGIN OF EARLY GALAXY r-PROCESS ELEMENTS?
3. Spectroscopic Studies of Extremely Metal-Poor Stars with the Subaru High Dispersion Spectrograph. II. The r-Process Elements, Including Thorium
4. Atomic Data and Nuclear Data Tables
5. New calculations of grossβ-decay properties for astrophysical applications: Speeding-up the classicalrprocess
6. Non-standard s process in low metallicity massive rotating stars
7. PRODUCTION OF ALL THE r-PROCESS NUCLIDES IN THE DYNAMICAL EJECTA OF NEUTRON STAR MERGERS
8. Neutron star mergers versus core-collapse supernovae as dominant r-process sites in the early Galaxy
9. r-PROCESS NUCLEOSYNTHESIS IN DYNAMICALLY EJECTED MATTER OF NEUTRON STAR MERGERS
10. Neutron-Capture Elements in the Very Metal Poor Star HD 122563

Their papers

• The Intermediate r-process in Core-collapse Supernovae Driven by the Magneto-rotational Instability (2016) — 135 citations