Optical photometry and spectroscopy of the 1987A-like supernova 2009mw

We present optical photometric and spectroscopic observations of the 1987A-like supernova (SN) 2009mw. Our BVRI and <i>g′r′i′z′</i> photometry covers 167 d of evolution, including the rise to the light-curve maximum, and ends just after the beginning of the linear tail phase. We compare...

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Autores principales: Takáts, K., Pignata, G., Bersten, Melina Cecilia, Rojas Kaufmann, María Luján, Anderson, J. P., Folatelli, Gastón, Hamuy, M., Stritzinger, M., Haislip, J. B., LaCluyze, A. P., Moore, J. P., Reichart, D.
Formato: Articulo Preprint
Lenguaje:Inglés
Publicado: 2016
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/93612
https://academic.oup.com/mnras/article-abstract/460/4/3447/2609043?redirectedFrom=fulltext
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id I19-R120-10915-93612
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Astronomía
Física
Ciencias Naturales
Ciencias Exactas
Supernovae
Evolution of stars
Hydrodynamics
SN 2009mw (supernova)
SN 1987A (supernova)
spellingShingle Astronomía
Física
Ciencias Naturales
Ciencias Exactas
Supernovae
Evolution of stars
Hydrodynamics
SN 2009mw (supernova)
SN 1987A (supernova)
Takáts, K.
Pignata, G.
Bersten, Melina Cecilia
Rojas Kaufmann, María Luján
Anderson, J. P.
Folatelli, Gastón
Hamuy, M.
Stritzinger, M.
Haislip, J. B.
LaCluyze, A. P.
Moore, J. P.
Reichart, D.
Optical photometry and spectroscopy of the 1987A-like supernova 2009mw
topic_facet Astronomía
Física
Ciencias Naturales
Ciencias Exactas
Supernovae
Evolution of stars
Hydrodynamics
SN 2009mw (supernova)
SN 1987A (supernova)
description We present optical photometric and spectroscopic observations of the 1987A-like supernova (SN) 2009mw. Our BVRI and <i>g′r′i′z′</i> photometry covers 167 d of evolution, including the rise to the light-curve maximum, and ends just after the beginning of the linear tail phase. We compare the observational properties of SN 2009mw with those of other SNe belonging to the same subgroup and find that it shows similarities to several objects. The physical parameters of the progenitor and the SN are estimated through hydrodynamical modelling, and yield an explosion energy of 1 foe, a pre-SN mass of 19 M⊙, a progenitor radius of 30 R⊙ and a <sup>56</sup>Ni mass of 0.062 M⊙. These values indicate that the progenitor of SN 2009mw was a blue supergiant star, similar to the progenitor of SN 1987A. We examine the host environment of SN 2009mw and find that it emerged from a population with a slightly subsolar metallicty.
format Articulo
Preprint
author Takáts, K.
Pignata, G.
Bersten, Melina Cecilia
Rojas Kaufmann, María Luján
Anderson, J. P.
Folatelli, Gastón
Hamuy, M.
Stritzinger, M.
Haislip, J. B.
LaCluyze, A. P.
Moore, J. P.
Reichart, D.
author_facet Takáts, K.
Pignata, G.
Bersten, Melina Cecilia
Rojas Kaufmann, María Luján
Anderson, J. P.
Folatelli, Gastón
Hamuy, M.
Stritzinger, M.
Haislip, J. B.
LaCluyze, A. P.
Moore, J. P.
Reichart, D.
author_sort Takáts, K.
title Optical photometry and spectroscopy of the 1987A-like supernova 2009mw
title_short Optical photometry and spectroscopy of the 1987A-like supernova 2009mw
title_full Optical photometry and spectroscopy of the 1987A-like supernova 2009mw
title_fullStr Optical photometry and spectroscopy of the 1987A-like supernova 2009mw
title_full_unstemmed Optical photometry and spectroscopy of the 1987A-like supernova 2009mw
title_sort optical photometry and spectroscopy of the 1987a-like supernova 2009mw
publishDate 2016
url http://sedici.unlp.edu.ar/handle/10915/93612
https://academic.oup.com/mnras/article-abstract/460/4/3447/2609043?redirectedFrom=fulltext
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