5.9-keV Mn K-shell X-ray luminosity from the decay of 55Fe in Type Ia supernova models
| dc.contributor.author | Seitenzahl, Ivo | |
| dc.contributor.author | Summa, A | |
| dc.contributor.author | Krauss, F. | |
| dc.contributor.author | Sim, Stuart | |
| dc.contributor.author | Diehl, R | |
| dc.contributor.author | Elsasser, D | |
| dc.contributor.author | Fink, M | |
| dc.contributor.author | Hillebrandt, Wolfgang | |
| dc.contributor.author | Kromer, M | |
| dc.contributor.author | Maeda, Keiichi | |
| dc.contributor.author | Mannheim, K | |
| dc.contributor.author | Seitenzahl, I. R. | |
| dc.contributor.author | Ruiter, A. J. | |
| dc.date.accessioned | 2015-12-10T23:16:31Z | |
| dc.date.issued | 2014 | |
| dc.date.updated | 2015-12-10T09:53:42Z | |
| dc.description.abstract | We 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.issn | 0035-8711 | |
| dc.identifier.uri | http://hdl.handle.net/1885/65096 | |
| dc.publisher | Blackwell Publishing Ltd | |
| dc.source | Monthly Notices of the Royal Astronomical Society | |
| dc.title | 5.9-keV Mn K-shell X-ray luminosity from the decay of 55Fe in Type Ia supernova models | |
| dc.type | Journal article | |
| local.bibliographicCitation.lastpage | 1490 | |
| local.bibliographicCitation.startpage | 1484 | |
| local.contributor.affiliation | Seitenzahl, Ivo, College of Physical and Mathematical Sciences, ANU | |
| local.contributor.affiliation | Summa, A, Universität Würzburg | |
| local.contributor.affiliation | Krauss, F., Universitat Wurzburg | |
| local.contributor.affiliation | Sim, Stuart, Queens University Belfast | |
| local.contributor.affiliation | Diehl, R, Max-Planck-Institut für extraterrestrische Physik | |
| local.contributor.affiliation | Elsasser, D, Universitat Wurzburg | |
| local.contributor.affiliation | Fink, M, Universitat Wurzburg | |
| local.contributor.affiliation | Hillebrandt, Wolfgang, Max Planck Institute for Astrophysics | |
| local.contributor.affiliation | Kromer, M, Max Planck Institut für Astrophysik | |
| local.contributor.affiliation | Maeda, Keiichi, University of Tokyo | |
| local.contributor.affiliation | Mannheim, K, Universität Würzburg | |
| local.contributor.affiliation | Seitenzahl, I. R., Max Planck Institut für Astrophysik | |
| local.contributor.affiliation | Ruiter, A. J., Max Planck Institut für Astrophysik | |
| local.contributor.authoruid | Seitenzahl, Ivo, u5472295 | |
| local.description.embargo | 2037-12-31 | |
| local.description.notes | Imported from ARIES | |
| local.identifier.absfor | 020100 - ASTRONOMICAL AND SPACE SCIENCES | |
| local.identifier.absseo | 970102 - Expanding Knowledge in the Physical Sciences | |
| local.identifier.ariespublication | a383154xPUB1051 | |
| local.identifier.citationvolume | 447 | |
| local.identifier.doi | 10.1093/mnras/stu2537 | |
| local.identifier.scopusID | 2-s2.0-84922513571 | |
| local.type.status | Published Version |