Creating White Dwarf Photospheres In The Laboratory
dc.contributor.utaustinauthor | Falcon, Ross E. | en |
dc.contributor.utaustinauthor | Winget, D. E. | en |
dc.contributor.utaustinauthor | Montgomery, M. H. | en |
dc.creator | Falcon, R. E. | en |
dc.creator | Rochau, G. A. | en |
dc.creator | Bailey, J. E. | en |
dc.creator | Ellis, J. L. | en |
dc.creator | Montgomery, M. H. | en |
dc.creator | Winget, D. E. | en |
dc.creator | Gomez, M. R. | en |
dc.creator | Leeper, R. J. | en |
dc.date.accessioned | 2015-04-16T14:47:54Z | en |
dc.date.available | 2015-04-16T14:47:54Z | en |
dc.date.issued | 2010-08 | en |
dc.description.abstract | We present a preliminary report from the laboratory astrophysics experiments to create macroscopic (similar to 19 cm(3)) hydrogen-plasmas with white dwarf (WD) photospheric conditions (i.e., temperature, electron density). These experiments, performed at the Z Pulsed Power Facility at Sandia National Laboratories, will serve as benchmarks for fundamental atomic line profile measurements in emission and absorption; they are targeted to address the discrepancy between theory and observation of WD photospheres - cooler photospheres in particular. | en |
dc.description.department | Astronomy | en |
dc.identifier.citation | Ross E. Falcon, G. A. Rochau, J. E. Bailey, J. L. Ellis, M. H. Montgomery, D. E. Winget, Matthew R. Gomez, R. J. Leeper. AIP Conference Proceedings 1273, 436 (Aug., 2010); doi: 10.1063/1.3527858 | en |
dc.identifier.doi | doi: 10.1063/1.3527858 | en |
dc.identifier.issn | 0094-243X | en |
dc.identifier.issn | 978-0-7354-0823-4 | en |
dc.identifier.uri | http://hdl.handle.net/2152/29439 | en |
dc.language.iso | English | en |
dc.relation.ispartofserial | 17th European White Dwarf Workshop | en_US |
dc.rights | Administrative deposit of works to UT Digital Repository: This works author(s) is or was a University faculty member, student or staff member; this article is already available through open access or the publisher allows a PDF version of the article to be freely posted online. The library makes the deposit as a matter of fair use (for scholarly, educational, and research purposes), and to preserve the work and further secure public access to the works of the University. | en |
dc.subject | white dwarfs | en |
dc.subject | methods: laboratory | en |
dc.subject | techniques: spectroscopic | en |
dc.subject | mass-distribution | en |
dc.subject | plasma | en |
dc.subject | stars | en |
dc.subject | sdss | en |
dc.subject | astronomy & astrophysics | en |
dc.title | Creating White Dwarf Photospheres In The Laboratory | en |
dc.type | Article | en |
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