Published July 20, 2012 | Version v1
Journal article

THREE-DIMENSIONAL EXPLOSION GEOMETRY OF STRIPPED-ENVELOPE CORE-COLLAPSE SUPERNOVAE. I. SPECTROPOLARIMETRIC OBSERVATIONS

  • 1. National Astronomical Observatory, Mitaka, Tokyo (Japan)
  • 2. Hiroshima Astrophysical Science Center, Hiroshima University, Higashi-Hiroshima, Hiroshima (Japan)
  • 3. Subaru Telescope, National Astronomical Observatory of Japan, Hilo, HI 96720 (United States)
  • 4. Max-Planck Institut für Astrophysik, Karl-Schwarzschild-Strasse 2 D-85748 Garching bei München (Germany)
  • 5. Institute for the Physics and Mathematics of the Universe, University of Tokyo, Kashiwa (Japan)
  • 6. Istituto Naz. di Astrofisica-Oss. Astron., Via Tiepolo, 11, 34131 Trieste (Italy)

Description

We study the multi-dimensional geometry of supernova (SN) explosions by means of spectropolarimetric observations of stripped-envelope SNe, i.e., SNe without a hydrogen-rich layer. We perform spectropolarimetric observations of two stripped-envelope SNe, Type Ib SN 2009jf and Type Ic SN 2009mi. Both objects show non-zero polarization at the wavelength of the strong lines. They also show a loop in the Stokes Q - U diagram, which indicates a non-axisymmetric, three-dimensional ion distribution in the ejecta. We show that five out of six stripped-envelope SNe, which have been observed spectropolarimetrically so far, show such a loop. This implies that a three-dimensional geometry is common in stripped-envelope SNe. We find that stronger lines tend to show higher polarization. This effect is not related to the geometry, and must be corrected for to compare the polarization of different lines or different objects. Even after the correction, however, there remains a dispersion of polarization degree among different objects. Such a dispersion might be caused by three-dimensional clumpy ion distributions viewed from different directions.

Availability note (English)

Available from http://dx.doi.org/10.1088/0004-637X/754/1/63

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
754
Journal Issue
1
Journal Page Range
[10 p.]
ISSN
0004-637X
CODEN
ASJOAB