Confirming chemical clocks: asteroseismic age dissection of the Milky Way disc(s)
- Submitting institution
-
University College London
- Unit of assessment
- 9 - Physics
- Output identifier
- 9868
- Type
- D - Journal article
- DOI
-
10.1093/mnras/sty150
- Title of journal
- MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
- Article number
- -
- First page
- 5487
- Volume
- 475
- Issue
- 4
- ISSN
- 0035-8711
- Open access status
- Compliant
- Month of publication
- January
- Year of publication
- 2018
- URL
-
-
- 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
-
24
- Research group(s)
-
-
- Citation count
- 62
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- -
- Author contribution statement
- Daisuke Kawata contributed to this paper on applying the novel asteroseismic age of the stars to Galactic chemodynamics studies, especially the results and discussion in Sec. 4.2. Kawata suggested Figs. 10 and 11 and analysed the kinematics of stars for these plots. Kawata also contributed to the interpretation and discussion from these results. Kawata suggested the discussion about kinematical properties of young ?-rich stars being similar to the old ?-rich stars, which infers that their origin is the same. This is one of the major results of this paper highlighted in abstract.
- Non-English
- No
- English abstract
- -