Mass-radius relation of low-mass stars from eclipsing binary stars.
Lead Research Organisation:
Keele University
Department Name: Faculty of Natural Sciences
Abstract
The project uses multiple data sources including TESS, K2, Xamidimura, and ground-based spectroscopy in order to parameterise lightcurves of eclipsing binaries and thence study the mass-radius relation of stars as a function of mass, metallicity, binary period, etc.
Organisations
People |
ORCID iD |
| Nicola Miller (Student) |
Studentship Projects
| Project Reference | Relationship | Related To | Start | End | Student Name |
|---|---|---|---|---|---|
| ST/N504348/1 | 30/09/2015 | 29/03/2021 | |||
| 2224078 | Studentship | ST/N504348/1 | 30/09/2018 | 29/09/2021 | Nicola Miller |
| ST/R504828/1 | 23/09/2018 | 22/09/2022 | |||
| 2224078 | Studentship | ST/R504828/1 | 30/09/2018 | 29/09/2021 | Nicola Miller |