TY - JOUR
T1 - Three-dimensional explosion geometry of stripped-envelope core-collapse supernovae. I. Spectropolarimetric observations
AU - Tanaka, Masaomi
AU - Kawabata, Koji S.
AU - Hattori, Takashi
AU - Mazzali, Paolo A.
AU - Aoki, Kentaro
AU - Iye, Masanori
AU - Maeda, Keiichi
AU - Nomoto, Ken'Ichi
AU - Pian, Elena
AU - Sasaki, Toshiyuki
AU - Yamanaka, Masayuki
PY - 2012/7/20
Y1 - 2012/7/20
N2 - 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.
AB - 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.
KW - supernovae: general
KW - supernovae: individual (SNe 2009jf, 2009mi)
KW - techniques: polarimetric
UR - http://www.scopus.com/inward/record.url?scp=84863662974&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84863662974&partnerID=8YFLogxK
U2 - 10.1088/0004-637X/754/1/63
DO - 10.1088/0004-637X/754/1/63
M3 - Article
AN - SCOPUS:84863662974
SN - 0004-637X
VL - 754
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 1
M1 - 63
ER -