ASYMMETRIES in SN 2014J NEAR MAXIMUM LIGHT REVEALED THROUGH SPECTROPOLARIMETRY

Amber L. Porter, Mark D. Leising, George G Williams, Peter Milne, Paul Smith, Nathan Smith, Christopher Bilinski, Jennifer L. Hoffman, Leah Huk, Douglas C. Leonard

Research output: Contribution to journalArticle

9 Citations (Scopus)

Abstract

We present spectropolarimetric observations of the nearby Type Ia supernova SN 2014J in M82 over six epochs: +0, +7, +23, +51, +77, +109, and +111 days with respect to B-band maximum. The strong continuum polarization, which is constant with time, shows a wavelength dependence unlike that produced by linear dichroism in Milky Way dust. The observed polarization may be due entirely to interstellar dust or include a circumstellar scattering component. We find that the polarization angle aligns with the magnetic field of the host galaxy, arguing for an interstellar origin. Additionally, we confirm a peak in polarization at short wavelengths that would imply RV < 2 along the light of sight, in agreement with earlier polarization measurements. For illustrative purposes, we include a two-component fit to the continuum polarization of our +51-day epoch that combines a circumstellar scattering component with interstellar dust where scattering can account for over half of the polarization at 4000 Å. Upon removal of the interstellar polarization signal, SN 2014J exhibits very low levels of continuum polarization. Asymmetries in the distribution of elements within the ejecta are visible through moderate levels of time-variable polarization in accordance with the Si II λ6355 absorption line. At maximum light, the line polarization reaches ∼0.6% and decreases to ∼0.4% 1 week later. This feature also forms a loop on the qRSP-uRSP plane, illustrating that the ion does not have an axisymmetric distribution. The observed polarization properties suggest that the explosion geometry of SN 2014J is generally spheroidal with a clumpy distribution of silicon.

Original languageEnglish (US)
Article number24
JournalAstrophysical Journal
Volume828
Issue number1
DOIs
StatePublished - Sep 1 2016

Fingerprint

polarization
dust
scattering
continuums
time measurement
wavelength
visual perception
ejecta
wavelengths
silicon
dichroism
supernovae
explosions
explosion
asymmetry
galaxies
magnetic field
geometry
ion
magnetic fields

Keywords

  • polarization
  • supernovae: general
  • supernovae: individual (SN 2014J)

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

ASYMMETRIES in SN 2014J NEAR MAXIMUM LIGHT REVEALED THROUGH SPECTROPOLARIMETRY. / Porter, Amber L.; Leising, Mark D.; Williams, George G; Milne, Peter; Smith, Paul; Smith, Nathan; Bilinski, Christopher; Hoffman, Jennifer L.; Huk, Leah; Leonard, Douglas C.

In: Astrophysical Journal, Vol. 828, No. 1, 24, 01.09.2016.

Research output: Contribution to journalArticle

Porter, AL, Leising, MD, Williams, GG, Milne, P, Smith, P, Smith, N, Bilinski, C, Hoffman, JL, Huk, L & Leonard, DC 2016, 'ASYMMETRIES in SN 2014J NEAR MAXIMUM LIGHT REVEALED THROUGH SPECTROPOLARIMETRY', Astrophysical Journal, vol. 828, no. 1, 24. https://doi.org/10.3847/0004-637X/828/1/24
Porter, Amber L. ; Leising, Mark D. ; Williams, George G ; Milne, Peter ; Smith, Paul ; Smith, Nathan ; Bilinski, Christopher ; Hoffman, Jennifer L. ; Huk, Leah ; Leonard, Douglas C. / ASYMMETRIES in SN 2014J NEAR MAXIMUM LIGHT REVEALED THROUGH SPECTROPOLARIMETRY. In: Astrophysical Journal. 2016 ; Vol. 828, No. 1.
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