Binary properties of Wolf-Rayet stars in nearby galaxies
Lead Research Organisation:
University of Sheffield
Department Name: Physics and Astronomy
Abstract
Wolf-Rayet stars are the evolved descendants of massive O and early B stars, and it has recently been recognised that a high fraction of massive stars are born in close binary systems. This project will focus on establishing binary properties of Wolf-Rayet stars in nearby galaxies spanning a range of metallicities, based on a mixture of optical spectroscopic datasets (primarily ground-based from 8-10m class telescopes for WR stars in other galaxies) and X-ray observations (from Chandra T-ReX programme). These approaches are complementary since optical observations are sensitive to Doppler shifts in close binaries whereas X-ray datasets focus on colliding wind systems which sample somewhat larger separations. Initial targets are IC10 (metal-poor draft galaxy in Local Group) and the Tarantula region in the LMC.
Organisations
Studentship Projects
Project Reference | Relationship | Related To | Start | End | Student Name |
---|---|---|---|---|---|
ST/N504282/1 | 01/10/2015 | 30/03/2021 | |||
1647894 | Studentship | ST/N504282/1 | 01/10/2015 | 01/04/2019 | Katayoun Abdollah-Tehrani |