NUGRID STELLAR DATA SET. I. STELLAR YIELDS FROM H TO BI FOR STARS WITH METALLICITIES
Z
= 0.02 and
Z
= 0.01
- Submitting institution
-
University of Keele
- Unit of assessment
- 9 - Physics
- Output identifier
- 296
- Type
- D - Journal article
- DOI
-
10.3847/0067-0049/225/2/24
- Title of journal
- The Astrophysical Journal Supplement Series
- Article number
- -
- First page
- 24
- Volume
- 225
- Issue
- 2
- ISSN
- 0067-0049
- Open access status
- Compliant
- Month of publication
- August
- Year of publication
- 2016
- URL
-
https://iopscience.iop.org/article/10.3847/0067-0049/225/2/24
- Supplementary information
-
-
- Request cross-referral to
- -
- Output has been delayed by COVID-19
- No
- COVID-19 affected output statement
- -
- Forensic science
- No
- Criminology
- No
- Interdisciplinary
- No
- Number of additional authors
-
18
- Research group(s)
-
-
- Citation count
- 85
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- Hirschi is one of the co-founders of the NuGrid international collaboration (https://nugrid.github.io/) involving 23 institutions across Europe, North America, Asia and Australia and was its PI for several separate years in the past 10 years. With his PhD student, Bennett, Hirschi developed a large part of the MPPNP code used in this study and calculated all the massive star evolution models used in this study with the GENEC code. Furthermore, Hirschi drafted text (e.g. Sections 2.1, 2.2, 3.1, 3.7.1) and created figures (13, 14) related to massive star evolution and nucleosynthesis throughout the paper.
- Author contribution statement
- -
- Non-English
- No
- English abstract
- -
