1995/10/02 by Peter Nugent, P. Nugent, Mark Phillips +5 · 11 citations
Chemistry · Physics and Astronomy · #Astro and Planetary Science #Astronomy #Astrophysics #Brightness #Chemistry #Gamma-ray bursts and supernovae #Geology #Light curve #Paleontology #Physics #Pulsars and Gravitational Waves Research #Sequence (biology) #Series (stratigraphy) #Spectral line #Supernova #Type (biology) #astro-ph
paper · pdf · doi:10.1086/309846
published as Astrophys.J.455:L147-L150,1995 · To appear in Astrophysical Journal Letters, uuencoded, gzipped postscript file, also available from http://www.nhn.uoknor.edu/~baron/
arxiv created 1995/10/02 · openalex publication_date 1995/12/20 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
In this Letter we present evidence for a spectral sequence among Type Ia supernovae (SN Ia's). The sequence is based on the systematic variation of several features seen in the near-maximum light spectrum. This sequence is analogous to the recently noted photometric sequence among SN Ia's which shows a relationship between the peak brightness of a SN Ia and the shape of its light curve. In addition to the observational evidence we present a partial theoretical explanation for the sequence. This has been achieved by producing a series of non-LTE synthetic spectra in which only the effective temperature is varied. The synthetic sequence nicely reproduces most of the differences seen in the observed one and presumably corresponds to the amount of 56 Ni produced in the explosion.