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BiBTeXDespite the importance of Type Ia supernovae for modern astrophysics, their detailed explosion mechanism is still not fully understood. In this article, we present recent findings from numerical models in the context of their observed diversity and we discuss how these models can help to shed light on the explosion mechanism and to identify their progenitor systems. It is shown that the models have considerable predictive power and they can aid the identification of sources of systematic errors when used as distance indicators for cosmology.
SEEK ID: https://publications.h-its.org/publications/410
Research Groups: Physics of Stellar Objects
Publication type: InProceedings
Book Title: NIC Symposium 2018
Publisher: Forschungszentrum Jülich GmbH, Zentralbibliothek
Citation: In NIC Symposium 2018, vol. 49 of NIC Series, pp. 99 - 106, Forschungszentrum Jülich GmbH, Zentralbibliothek, Jülich
Date Published: 1st Feb 2018
Registered Mode: imported from a bibtex file
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Created: 7th Sep 2019 at 12:23
Last updated: 5th Mar 2024 at 21:23
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Research Groups: Physics of Stellar Objects
Institutions: Heidelberg Institute for Theoretical Studies
https://orcid.org/0000-0002-4460-0097
Research Groups: Scientific Databases and Visualisation, Astroinformatics, Data Mining and Uncertainty Quantification, Groups and Geometry, Natural Language Processing, Computational Molecular Evolution, Computational Carbon Chemistry, Physics of Stellar Objects, Playground, Molecular and Cellular Modeling, Stellar Evolution Theory, SIMPLAIX
Institutions: Heidelberg Institute for Theoretical Studies
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