1. Two transitional type Ia supernovae located in the Fornax cluster member NGC 1404: SN 2007on and SN 2011iv
- Author
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Francesco Taddia, Yen-Chen Pan, S. Holmbo, Peter J. Brown, G. Folatelli, Giuliano Pignata, Alexei V. Filippenko, Peter Hoeflich, E. Baron, George H Marion, Stefano Benetti, S. Torres Robledo, Mark M. Phillips, R. J. Foley, Maximilian Stritzinger, Nidia Morrell, Nicholas B. Suntzeff, Christopher R. Burns, Carlos Contreras, Paolo A. Mazzali, Eric Hsiao, Chris Ashall, Christa Gall, N. Elias de la Rosa, Stefano Valenti, Joseph P. Anderson, Abdo Campillay, Morgan Fraser, and P. Challis
- Subjects
Individual: Sn 2007on [Supernovae] ,Ciencias Físicas ,Supernovae individual SN 2011iv ,DELAYED-DETONATION MODEL ,Astrophysics ,01 natural sciences ,THERMONUCLEAR SUPERNOVAE ,Luminosity ,Dust, Extinction ,purl.org/becyt/ford/1 [https] ,ULTRAVIOLET-SPECTRA ,NEAR-INFRARED OBSERVATIONS ,CHANDRASEKHAR-MASS MODELS ,Fornax Cluster ,010303 astronomy & astrophysics ,QC ,QB ,High Energy Astrophysical Phenomena (astro-ph.HE) ,astro-ph.HE ,Physics ,Dust ,Extinction ,Individual: Sn 2011iv [Supernovae] ,Supernova ,Astrophysics - Solar and Stellar Astrophysics ,Transition density ,ASYMMETRIC EXPLOSION ,Astrophysics - High Energy Astrophysical Phenomena ,CIENCIAS NATURALES Y EXACTAS ,astro-ph.SR ,FOS: Physical sciences ,Context (language use) ,0103 physical sciences ,Ciencias Naturales ,general individual SN 2007on [Supernovae] ,Solar and Stellar Astrophysics (astro-ph.SR) ,Ciencias Exactas ,LIGHT CURVES ,General [Supernovae] ,010308 nuclear & particles physics ,ACCRETING WHITE-DWARFS ,Física ,White dwarf ,LUMINOSITY INDICATORS ,Astronomy and Astrophysics ,purl.org/becyt/ford/1.3 [https] ,Light curve ,First order ,Astronomía ,Space and Planetary Science ,Supernovae: general individual SN 2007on ,SURFACE BRIGHTNESS FLUCTUATIONS - Abstract
We present an analysis of ultraviolet (UV) to near-infrared observations of the fast-declining Type Ia supernovae (SNe Ia) 2007on and 2011iv, hosted by the Fornax cluster member NGC 1404. The B-band light curves of SN 2007on and SN 2011iv are characterised by Δm15 (B) decline-rate values of 1.96 mag and 1.77 mag, respectively. Although they have similar decline rates, their peak B- and H-band magnitudes differ by ~ 0.60 mag and ~0.35 mag, respectively. After correcting for the luminosity vs. decline rate and the luminosity vs. colour relations, the peak B-band and H-band light curves provide distances that differ by ~ 14% and ~ 9%, respectively. These findings serve as a cautionary tale for the use of transitional SNe Ia located in early-type hosts in the quest to measure cosmological parameters. Interestingly, even though SN 2011iv is brighter and bluer at early times, by three weeks past maximum and extending over several months, its B - V colour is 0.12 mag redder than that of SN 2007on. To reconcile this unusual behaviour, we turn to guidance from a suite of spherical one-dimensional Chandrasekhar-mass delayed-detonation explosion models. In this context, 56Ni production depends on both the so-called transition density and the central density of the progenitor white dwarf. To first order, the transition density drives the luminosity-width relation, while the central density is an important second-order parameter. Within this context, the differences in the B - V colour evolution along the Lira regime suggest that the progenitor of SN 2011iv had a higher central density than SN 2007on., Instituto de Astrofísica de La Plata, Facultad de Ciencias Astronómicas y Geofísicas
- Published
- 2018