Spectral luminosity indicators in SNe Ia - Understanding the R(SiII) line strength ratio and beyond

Details Spectral luminosity indicators in SNe Ia - Understanding the R(SiII) line strength ratio and beyond Spectral luminosity indicators in SNe Ia - Understanding the R(SiII) line strength ratio and beyond

2008-06-25

arxiv.org/abs/0806.4177v1

Mon.Not.Roy.Astron.Soc.389:1087-1096,2008

Astronomy and Astrophysics

Astrophysics

10 pages, 16 figures. Accepted for publication in MNRAS

Scientific paper

10.1063/1.3141612

SNe Ia are good distance indicators because the shape of their light curves, which can be measured independently of distance, varies smoothly with luminosity. This suggests that SNe Ia are a single family of events. Similar correlations are observed between luminosity and spectral properties. In particular, the ratio of the strengths of the SiII \lambda 5972 and \lambda 6355 lines, known as R(SiII), was suggested as a potential luminosity indicator. Here, the physical reasons for the observed correlation are investigated. A Monte-Carlo code is used to construct a sequence of synthetic spectra resembling those of SNe with different luminosities near B maximum. The influence of abundances and of ionisation and excitation conditions on the synthetic spectral features is investigated. The ratio R(SiII) depends ssentially on the strength of SiII \lambda 5972, because SiII \lambda 6355 is saturated. In less luminous objects, SiII \lambda 5972 is stronger because of a rapidly increasing SiII/SiIII ratio. Thus, the correlation between R(SiII) and luminosity is the effect of ionisation balance. The SiII \lambda 5972 line itself may be the best spectroscopic luminosity indicator for SNe Ia, but all indicators discussed show scatter which may be related to abundance distributions.

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