M. Aikawa
Astronomy and Astrophysics · 2004–2014
A researcher in the Science corpus: 3 papers; trusts 1 researcher and is trusted by 5 researchers here, as inferred from the citation graph.
Subfields
- Astronomy and Astrophysics — 33 citations into it; #7,393 of 10,964 by trust here, #6,524 by citations
Whom M. Aikawa trusts overall
Their strongest outbound trust, strongest first, inferred from their citations.
Who trusts M. Aikawa overall
Papers from M. Aikawa's perspective
Ordered by how strongly the researchers M. Aikawa trusts endorse each paper. Same corpus, a different order for every researcher.
- THE DISCOVERY AND ANALYSIS OF VERY METAL-POOR STARS IN THE GALAXY
- First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy
- Abundances of 30 Elements in 23 Metal-Poor Stars
- A Subaru/High Dispersion Spectrograph Study of Lead (Pb) Abundances in Eight s-Process Element-rich, Metal-poor Stars
- Spectroscopic Studies of Very Metal-poor Stars with the Subaru High Dispersion Spectrograph. III. Light Neutron-Capture Elements
- HE 0107–5240, a Chemically Ancient Star. I. A Detailed Abundance Analysis
- First stars. I. The extreme r-element rich, iron-poor halo giant CS 31082-001 - Implications for the r-process site(s) and radioactive cosmochronology
- Carbon-enhanced Metal-poor Stars. I. Chemical Compositions of 26 Stars
- Neutron Capture Elements in s-Process-Rich, Very Metal-Poor Stars
- Is HE 0107–5240 A Primordial Star? The Characteristics of Extremely Metal-Poor Carbon-Rich Stars
Their papers
- Stellar Abundances for the Galactic Archeology (SAGA) Database — Compilation of the Characteristics of Known Extremely Metal-Poor Stars (2008) — 337 citations
- Towards a More Complete and Accurate Experimental Nuclear Reaction Data Library (EXFOR): International Collaboration Between Nuclear Reaction Data Centres (NRDC) (2014) — 855 citations
- Is HE 0107–5240 A Primordial Star? The Characteristics of Extremely Metal-Poor Carbon-Rich Stars (2004) — 173 citations