Journal article
Ultraviolet spectropolarimetric diagnostics of hot star magnetospheres
Astrophysics and space science, Vol.367(12), p.117
12/01/2022
DOI: 10.1007/s10509-022-04097-8
Abstract
Several space missions and instruments for UV spectropolarimetry are in preparation, such as the proposed NASA MIDEX
Polstar
project, the proposed ESA M mission Arago, and the Pollux instrument on the future LUVOIR-like NASA flagship mission. In the frame of
Polstar
, we have studied the capabilities these observatories would offer to gain information on the magnetic and plasma properties of the magnetospheres of hot stars, helping us test the fundamental hypothesis that magnetospheres should act to rapidly drain angular momentum, thereby spinning the star down, whilst simultaneously reducing the net mass-loss rate. Both effects are expected to lead to dramatic differences in the evolution of magnetic vs. non-magnetic stars.
Details
- Title: Subtitle
- Ultraviolet spectropolarimetric diagnostics of hot star magnetospheres
- Creators
- A. ud-Doula - University of ScrantonM. C. M. Cheung - Lockheed Martin (United States)A. David-Uraz - Astrophysics Science DivisionC. Erba - East Tennessee State UniversityC. P. Folsom - Tartu ObservatoryK. Gayley - University of IowaY. Nazé - University of LiègeC. Neiner - Laboratoire d’études spatiales et d’instrumentation en astrophysiqueV. Petit - University of DelawareR. Prinja - UK Astronomy Technology CentreM. E. Shultz - University of DelawareN. Sudnik - Nicolaus Copernicus Astronomical CenterJ. S. Vink - Armagh Observatory & PlanetariumG. A. Wade - Royal Military College of Canada
- Resource Type
- Journal article
- Publication Details
- Astrophysics and space science, Vol.367(12), p.117
- DOI
- 10.1007/s10509-022-04097-8
- ISSN
- 0004-640X
- eISSN
- 1572-946X
- Publisher
- Springer Netherlands
- Grant note
- TM1-22001B; GO2-23003X / National Aeronautics and Space Administration (http://dx.doi.org/10.13039/100000104)
- Language
- English
- Date published
- 12/01/2022
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984429040802771
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