Evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates for LIGO/Virgo binary black holes
- Submitting institution
-
University of Keele
- Unit of assessment
- 9 - Physics
- Output identifier
- 292
- Type
- D - Journal article
- DOI
-
10.1051/0004-6361/201936528
- Title of journal
- Astronomy & Astrophysics
- Article number
- A104
- First page
- -
- Volume
- 636
- Issue
- -
- ISSN
- 0004-6361
- Open access status
- Compliant
- Month of publication
- April
- Year of publication
- 2020
- URL
-
https://www.aanda.org/articles/aa/abs/2020/04/aa36528-19/aa36528-19.html
- 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
-
33
- Research group(s)
-
-
- Citation count
- 55
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- "Hirschi was part of the 2 teams (“Geneva” and “MESA”) calculating the
stellar evolution model grids used in this study. The Geneva team has
been calculating one the largest and most used grids of rotating
models. The “MESA” team (Hirschi, Jones and Fields) calculated (with
the MESA code) the new grid of magnetic models published in this
study. Furthermore, Hirschi analysed and compared the 2 grids (MESA
versus GENEC; magnetic versus non-magnetic) and drafted several
sections of the paper: Sect. 4.1, sections 6.1 and 6.2. With his PhD
student, Kaiser, Hirschi also calculated additional models for figure
28."
- Author contribution statement
- -
- Non-English
- No
- English abstract
- -
