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Signatures of Delayed Detonation, Asymmetry, and Electron Capture in the Mid-Infrared Spectra of Supernovae 2003hv and 2005df
Vise andre og tillknytning
2007 (engelsk)Inngår i: The Astrophysical Journal, Vol. 661, nr 2, s. 995-1012Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

We present mid-infrared (5.2-15.2 μm) spectra of the Type Ia supernovae (SNe Ia) 2003hv and 2005df observed with the Spitzer Space Telescope. These are the first observed mid-infrared spectra of thermonuclear supernovae, and show strong emission from fine-structure lines of Ni, Co, S, and Ar. The detection of Ni emission in SN 2005df 135 days after the explosion provides direct observational evidence of high-density nuclear burning forming a significant amount of stable Ni in a SN Ia. The SN 2005df Ar lines also exhibit a two-pronged emission profile, implying that the Ar emission deviates significantly from spherical symmetry. The spectrum of SN 2003hv also shows signs of asymmetry, exhibiting blueshifted [Co III], which matches the blueshift of [Fe II ] lines in nearly coeval near-infrared spectra. Finally, local thermodynamic equilibrium abundance estimates for the yield of radioactive 56Ni give M56Ni~0.5 Msolar, for SN 2003hv, but only M56Ni~0.13-0.22 Msolar for the apparently subluminous SN 2005df, supporting the notion that the luminosity of SNe Ia is primarily a function of the radioactive 56Ni yield. The observed emission-line profiles in the SN 2005df spectrum indicate a chemically stratified ejecta structure, which matches the predictions of delayed detonation (DD) models, but is entirely incompatible with current three-dimensional deflagration models. Furthermore, the degree that this layering persists to the innermost regions of the supernova is difficult to explain even in a DD scenario, where the innermost ejecta are still the product of deflagration burning. Thus, while these results are roughly consistent with a delayed detonation, it is clear that a key piece of physics is still missing from our understanding of the earliest phases of SN Ia explosions.

sted, utgiver, år, opplag, sider
2007. Vol. 661, nr 2, s. 995-1012
Emneord [en]
Stars: Supernovae: General, supernovae: individual (SN 2003hv), supernovae: individual (SN 2005df)
HSV kategori
Identifikatorer
URN: urn:nbn:se:su:diva-11942DOI: doi:10.1086/516728OAI: oai:DiVA.org:su-11942DiVA, id: diva2:178461
Tilgjengelig fra: 2008-01-14 Laget: 2008-01-14 Sist oppdatert: 2011-01-11bibliografisk kontrollert

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