Million Degree Plasmas in Extreme Ultraviolet (EUV) Astrophysics

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dc.creatorKowalski, Michael P.
dc.creatorBarstow, Martin
dc.creatorBruhweiler, Frederick
dc.creatorCruddace, Raymond
dc.creatorDupree, Andrea
dc.creatorHolberg, Jay
dc.creatorHowell, Steve
dc.creatorLaming, J. Martin
dc.creatorLinsky, Jeffrey
dc.creatorSion, Edward
dc.creatorStrohmayer, Tod
dc.creatorSzkody, Paula
dc.creatorWelsh, Barry
dc.creatorWolff, Michael
dc.creatorWood, Kent
dc.date2009-03-30
dc.date.accessioned2026-07-07T12:58:10Z
dc.date.available2026-07-07T12:58:10Z
dc.descriptionMillion degree plasmas are ubiquitous in the Universe, and examples include the atmospheres of white dwarfs; accretion phenomena in young stars, cataclysmic variables and active galactic nuclei; the coronae of stars; and the interstellar medium of our own galaxy and of others. The bulk of radiation from million degree plasmas is emitted at extreme ultraviolet (EUV) wavelengths, which includes critical spectral features containing diagnostic information often not available at other wavelengths. With underpinning by a mature instrument technology, there is great opportunity here for exciting discoveries.
dc.description8 pages, 3 figures; Science White Paper for the Astro2010 decadal review
dc.identifierhttps://arxiv.org/abs/0903.5212
dc.identifierhttp://arxiv.org/abs/0903.5212
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/225153
dc.subjectAstrophysics of Galaxies
dc.subjectSolar and Stellar Astrophysics
dc.titleMillion Degree Plasmas in Extreme Ultraviolet (EUV) Astrophysics
dc.typetext

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