Astronomy Thesis Collection
Published December 5, 2023 | Version v1
Thesis Open

Study of the diversity of type Ia supernova progenitors

Authors/Creators

  • 1. A I Alikhanyan National Science Laboratory

Contributors

Supervisor:

  • 1. A I Alikhanyan National Science Laboratory

Description

The thesis is devoted to the investigation of the diversity of type Ia supernovae (SNe) progenitors. First of all we present an analysis of the height distributions of the different types of SNe from the plane of their host galaxies. We use a well-defined sample of 102 nearby SNe appearing inside high-inclined (i ≥ 85 deg), morphologically non-disturbed S0-Sd host galaxies from the Sloan Digital Sky Survey. Then, in the next chapter, using spectroscopically classified normal, 91T-, and 91bg-like 197 SNe Ia, we perform an analysis of their height distributions from the disc in edge-on spirals and investigate their light-curve (LC) decline rates (∆m15).
After this, we present an analysis of the LC decline rates of 407 normal and peculiar SNe Ia and global parameters of their host galaxies. Next, we perform an analysis of the galactocentric distributions of the normal and peculiar 91bg-like subclasses of 109 SNe Ia, and study the global parameters of their elliptical hosts.
To perform various comparisons between the properties/numbers of the different subsamples, we use the well-known statistical tests (Kolmogorov-Smirnov and Anderson-Darling tests, etc.) with the implementation of the WOLFRAM MATHEMATICA software and Monte Carlo simulations. In addition to the mentioned tests, we use the Kendall's and Spearman's rank coefficients/tests to analyse the possible correlations between the physical (intrinsic) properties of SNe Ia (subclass, ∆m15, etc.) and their host galaxies (stellar mass, age, etc.).
Our investigation of SNe Ia LC decline rates at different locations within their host galaxies aided in distinguishing between SNe Ia with young progenitors (slow-decliners), corresponding to the "prompt" component with short delay times, and those (fast-decliners) with "older" components exhibiting long delay times. The observational findings are in line with the SN Ia explosion models involving a sub-MCh mass white dwarf, where the SN LC decline rate serves as a suitable indicator of progenitor population age.

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