Very regular high-frequency pulsation modes in young intermediate-mass stars
- Submitting institution
-
University of Keele
- Unit of assessment
- 9 - Physics
- Output identifier
- 307
- Type
- D - Journal article
- DOI
-
10.1038/s41586-020-2226-8
- Title of journal
- Nature
- Article number
- -
- First page
- 147
- Volume
- 581
- Issue
- 7807
- ISSN
- 0028-0836
- Open access status
- Compliant
- Month of publication
- May
- Year of publication
- 2020
- URL
-
https://www.nature.com/articles/s41586-020-2226-8
- 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
-
35
- Research group(s)
-
-
- Citation count
- 8
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- Smalley (as a spectroscopy expert within the TESS Asteroseismic Science Consortium [TASC] working group WG-4 on A-F stars), determined the projected stellar rotational velocities (vsini), as listed in Extended Data Table 2, by using high-resolution stellar spectra and spectrum synthesis techniques as described in Methods: High-resolution spectroscopy. He also provided the independent Teff determinations using the infrared flux method, as used in Methods: Fundamental stellar properties.
- Author contribution statement
- -
- Non-English
- No
- English abstract
- -
