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Ultraviolet spectropolarimetric diagnostics of hot star magnetospheres

dc.contributorPenn State Scranton, 120 Ridge View Drive, 18512, Dunmore, PA, USA
dc.contributorLockheed Martin Solar and Astrophysics Laboratory, 3251 Hanover St, 94304, Palo Alto, CA, USA
dc.contributorDepartment of Physics and Astronomy, Howard University, 20059, Washington, DC, USA; Center for Research and Exploration in Space Science and Technology, and X-ray Astrophysics Laboratory, NASA/GSFC, 20771, Greenbelt, MD, USA; Center for Research and Exploration in Space Science and Technology, and X-ray Astrophysics Laboratory, NASA/GSFC, 20771, Greenbelt, MD, USA
dc.contributorDepartment of Physics & Astronomy, East Tennessee State University, 37614, Johnson City, TN, USA
dc.contributorTartu Observatory, University of Tartu, Observatooriumi 1, 61602, Toravere, Estonia
dc.contributorDepartment of Physics & Astronomy, University of Iowa, 203 Van Allen Hall, 52242, Iowa City, IA, USA
dc.contributorGAPHE, Université de Liège, Allée du 6 Août 19c (B5C), B-4000, Liège, Sart Tilman, Belgium
dc.contributorLESIA, Paris Observatory, PSL University, CNRS, Sorbonne University, Université de Paris, 5 place Jules Janssen, 92195, Meudon, France
dc.contributorDepartment of Physics and Astronomy, University of Delaware, 217 Sharp Lab, 19716, Newark, DE, USA
dc.contributorDepartment of Physics and Astronomy, Gower Street, WC1E 6BT, London, UK
dc.contributorNicolaus Copernicus Astronomical Centre of the Polish Academy of Sciences, Bartycka 18, 00-716, Warsaw, Poland
dc.contributorArmagh Observatory and Planetarium, College Hill, BT61 9DG, Armagh, Northern Ireland, UK
dc.contributorDepartment of Physics and Space Science, Royal Military College of Canada, PO Box 17000, Station Forces, K7K 7B4, Kingston, ON, Canada
dc.contributor.authorud-Doula, A.
dc.contributor.authorCheung, M. C. M.
dc.contributor.authorDavid-Uraz, A.
dc.contributor.authorErba, C.
dc.contributor.authorFolsom, C. P.
dc.contributor.authorGayley, K.
dc.contributor.authorNazé, Y.
dc.contributor.authorNeiner, C.
dc.contributor.authorPetit, V.
dc.contributor.authorPrinja, R.
dc.contributor.authorShultz, M. E.
dc.contributor.authorSudnik, N.
dc.contributor.authorVink, J. S.
dc.contributor.authorWade, G. A.
dc.date.accessioned2024-02-21T11:02:55Z
dc.date.available2024-02-21T11:02:55Z
dc.date.issued2022-12-01T00:00:00Z
dc.identifier.doi10.1007/s10509-022-04097-8
dc.identifier.doi10.48550/arXiv.2206.12838
dc.identifier.other2022arXiv220612838U
dc.identifier.otherastro-ph.SR
dc.identifier.other2022arXiv220612838U
dc.identifier.other2022Ap&SS.367..117U
dc.identifier.other10.1007/s10509-022-04097-8
dc.identifier.other10.48550/arXiv.2206.12838
dc.identifier.otherarXiv:2206.12838
dc.identifier.other0000-0001-7721-6713
dc.identifier.other-
dc.identifier.urihttp://hdl.handle.net/20.500.14302/1708
dc.description.abstractSeveral 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.
dc.publisherAstrophysics and Space Science
dc.titleUltraviolet spectropolarimetric diagnostics of hot star magnetospheres
dc.typearticle
dc.source.journalAp&SS
dc.source.journalAp&SS.367
dc.source.volume367
refterms.dateFOA2024-02-21T11:02:55Z
dc.identifier.bibcode2022Ap&SS.367..117U


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