The early phases of the type Iax supernova SN 2011ay

Tamás Szalai, J. Vinkó, Krisztián Sárneczky, Katalin Takáts, J. Benkő, János Kelemen, Zoltán Kuli, Jeffrey M. Silverman, G. Howie Marion, J. Craig Wheeler

Research output: Contribution to journalArticle

8 Citations (Scopus)

Abstract

We present a detailed study of the early phases of the peculiar supernova (SN) 2011ay based on BVRI photometry obtained at Konkoly Observatory, Hungary, and optical spectra taken with the Hobby-Eberly Telescope at McDonald Observatory, Texas. The spectral analysis carried out with SYN++ and SYNAPPS confirms that SN 2011ay belongs to the recently defined class of SNe Iax, which is also supported by the properties of its light and colour curves. The estimated photospheric temperature around maximum light, Tphot ~8000 K, is lower than in most SNe Ia, which results in the appearance of strong Fe II features in the spectra of SN 2011ay, even during the early phases. We also show that strong blending with metal features (those of Ti II, FeII, Co II) makes the direct analysis of the broad spectral features very difficult, and this may be true for all SNe Iax. We find two alternative spectrum models that both describe the observed spectra adequately, but their photospheric velocities differ by at least ~3000 km s-1. The quasi-bolometric light curve of SN 2011ay has been assembled by integrating the ultraviolet-optical spectral energy distributions. Fitting a modified Arnett model to Lbol(t), the moment of explosion and other physical parameters, i.e. the rise time to maximum, the 56Ni mass and the total ejecta mass are estimated as trise ~ 14 ± 1 d, MNi ~ 0.22 ± 0.01M⊙ and Mej ~ 0.8M⊙, respectively.

Original languageEnglish
Pages (from-to)2103-2114
Number of pages12
JournalMonthly Notices of the Royal Astronomical Society
Volume453
Issue number2
DOIs
Publication statusPublished - Aug 6 2015

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supernovae
observatory
light curve
observatories
Hungary
ejecta
spectral analysis
explosion
spectral energy distribution
spectrum analysis
photometry
explosions
optical spectrum
telescopes
metal
moments
color
energy
curves
temperature

Keywords

  • Supernovae: general
  • Supernovae: individual: SN 2011ay

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

The early phases of the type Iax supernova SN 2011ay. / Szalai, Tamás; Vinkó, J.; Sárneczky, Krisztián; Takáts, Katalin; Benkő, J.; Kelemen, János; Kuli, Zoltán; Silverman, Jeffrey M.; Howie Marion, G.; Craig Wheeler, J.

In: Monthly Notices of the Royal Astronomical Society, Vol. 453, No. 2, 06.08.2015, p. 2103-2114.

Research output: Contribution to journalArticle

Szalai, T, Vinkó, J, Sárneczky, K, Takáts, K, Benkő, J, Kelemen, J, Kuli, Z, Silverman, JM, Howie Marion, G & Craig Wheeler, J 2015, 'The early phases of the type Iax supernova SN 2011ay', Monthly Notices of the Royal Astronomical Society, vol. 453, no. 2, pp. 2103-2114. https://doi.org/10.1093/mnras/stv1776
Szalai, Tamás ; Vinkó, J. ; Sárneczky, Krisztián ; Takáts, Katalin ; Benkő, J. ; Kelemen, János ; Kuli, Zoltán ; Silverman, Jeffrey M. ; Howie Marion, G. ; Craig Wheeler, J. / The early phases of the type Iax supernova SN 2011ay. In: Monthly Notices of the Royal Astronomical Society. 2015 ; Vol. 453, No. 2. pp. 2103-2114.
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AU - Benkő, J.

AU - Kelemen, János

AU - Kuli, Zoltán

AU - Silverman, Jeffrey M.

AU - Howie Marion, G.

AU - Craig Wheeler, J.

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