Cultural advice

The Australian National University acknowledges, celebrates and pays our respects to the Ngunnawal and Ngambri people of the Canberra region and to all First Nations Australians on whose traditional lands we meet and work, and whose cultures are among the oldest continuing cultures in human history.

Aboriginal and Torres Strait Islander peoples are advised that ANU Library collections may include images, names, voices, and other representations of deceased persons.

Material in the collection may contain terms, language or views that reflect the period in which the item was created and may be considered inappropriate today.

5.9-keV Mn K-shell X-ray luminosity from the decay of 55Fe in Type Ia supernova models

dc.contributor.authorSeitenzahl, Ivo
dc.contributor.authorSumma, A
dc.contributor.authorKrauss, F.
dc.contributor.authorSim, Stuart
dc.contributor.authorDiehl, R
dc.contributor.authorElsasser, D
dc.contributor.authorFink, M
dc.contributor.authorHillebrandt, Wolfgang
dc.contributor.authorKromer, M
dc.contributor.authorMaeda, Keiichi
dc.contributor.authorMannheim, K
dc.contributor.authorSeitenzahl, I. R.
dc.contributor.authorRuiter, A. J.
dc.date.accessioned2015-12-10T23:16:31Z
dc.date.issued2014
dc.date.updated2015-12-10T09:53:42Z
dc.description.abstractWe show that the X-ray line flux of the Mn Kα line at 5.9 keV from the decay of 55Fe is a promising diagnostic to distinguish between Type Ia supernova (SN Ia) explosion models. Using radiation transport calculations, we compute the line flux for two thr
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/65096
dc.publisherBlackwell Publishing Ltd
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.title5.9-keV Mn K-shell X-ray luminosity from the decay of 55Fe in Type Ia supernova models
dc.typeJournal article
local.bibliographicCitation.lastpage1490
local.bibliographicCitation.startpage1484
local.contributor.affiliationSeitenzahl, Ivo, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSumma, A, Universität Würzburg
local.contributor.affiliationKrauss, F., Universitat Wurzburg
local.contributor.affiliationSim, Stuart, Queens University Belfast
local.contributor.affiliationDiehl, R, Max-Planck-Institut für extraterrestrische Physik
local.contributor.affiliationElsasser, D, Universitat Wurzburg
local.contributor.affiliationFink, M, Universitat Wurzburg
local.contributor.affiliationHillebrandt, Wolfgang, Max Planck Institute for Astrophysics
local.contributor.affiliationKromer, M, Max Planck Institut für Astrophysik
local.contributor.affiliationMaeda, Keiichi, University of Tokyo
local.contributor.affiliationMannheim, K, Universität Würzburg
local.contributor.affiliationSeitenzahl, I. R., Max Planck Institut für Astrophysik
local.contributor.affiliationRuiter, A. J., Max Planck Institut für Astrophysik
local.contributor.authoruidSeitenzahl, Ivo, u5472295
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
local.identifier.ariespublicationa383154xPUB1051
local.identifier.citationvolume447
local.identifier.doi10.1093/mnras/stu2537
local.identifier.scopusID2-s2.0-84922513571
local.type.statusPublished Version

Downloads

Original bundle

Now showing 1 - 2 of 2
Loading...
Thumbnail Image
Name:
01_Seitenzahl_5.9-keV_Mn_K-shell_X-ray_2014.pdf
Size:
389.09 KB
Format:
Adobe Portable Document Format
Loading...
Thumbnail Image
Name:
02_Seitenzahl_5.9-keV_Mn_K-shell_X-ray_2014.pdf
Size:
127.96 KB
Format:
Adobe Portable Document Format