Study of Supernovae Important for Cosmology

The dense shell method for the determination of distances to type IIn supernovae has been briefly reviewed. Applying our method to SN 2006gy, SN 2009ip, and SN 2010jl supernovae, we have obtained distances in excellent agreement with the previously known distances to the parent galaxies. The dense s...

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Veröffentlicht in:arXiv.org 2015-02
Hauptverfasser: Baklanov, P V, Blinnikov, S I, M Sh Potashov, Dolgov, A D
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Blinnikov, S I
M Sh Potashov
Dolgov, A D
description The dense shell method for the determination of distances to type IIn supernovae has been briefly reviewed. Applying our method to SN 2006gy, SN 2009ip, and SN 2010jl supernovae, we have obtained distances in excellent agreement with the previously known distances to the parent galaxies. The dense shell method is based on the radiation hydrodynamic model of a supernova. The method of the blackbody model, as well as the correctness of its application for simple estimates of distances from observation data, has been justified.
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subjects Blackbody
Cosmology
Galaxies
Physics - Cosmology and Nongalactic Astrophysics
Physics - High Energy Astrophysical Phenomena
Physics - High Energy Physics - Phenomenology
Supernovae
title Study of Supernovae Important for Cosmology
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