VLT spectropolarimetry of the fast expanding type Ia SN 2006X

F. Patat; D. Baade; P. Höflich; J. R. Maund; L. Wang; J. C. Wheeler

doi:10.1051/0004-6361/200810651

Free Access

Issue		A&A Volume 508, Number 1, December II 2009


Page(s)		229 - 246
Section		Interstellar and circumstellar matter
DOI		https://doi.org/10.1051/0004-6361/200810651
Published online		01 October 2009

Online Material

Appendix A: Additional figures

$\begin{figure} \includegraphics[width=10cm]{10651f28.eps} \end{figure}$	Figure A.1: Spectropolarimetric data for SN 2006X on day -10. From top to bottom: total flux spectrum (in 10^-15 erg s^-1cm^-2 Å^-1), ISP corrected polarization degree, the Stokes parameters Q and U and polarization position angle on the plane of the sky.
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$\begin{figure} \par\includegraphics[width=10cm]{10651f29.eps} \end{figure}$	Figure A.2: Same as Fig. A.1 for day -8.
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$\begin{figure} \par\includegraphics[width=10cm]{10651f30.eps} \end{figure}$	Figure A.3: Same as Fig. A.1 for day -7.
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$\begin{figure} \par\includegraphics[width=10cm]{10651f31.eps} \end{figure}$	Figure A.4: Same as Fig. A.1 for day -6.
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$\begin{figure} \par\includegraphics[width=10cm]{10651f32.eps} \end{figure}$	Figure A.5: Same as Fig. A.1 for day -3.
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$\begin{figure} \par\includegraphics[width=10cm]{10651f33.eps} \end{figure}$	Figure A.6: Same as Fig. A.1 for day -2.
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$\begin{figure} \par\includegraphics[width=10cm]{10651f34.eps} \end{figure}$	Figure A.7: Same as Fig. A.1 for day -1.
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$\begin{figure} \par\includegraphics[width=10cm]{10651f35.eps} \end{figure}$	Figure A.8: Same as Fig. A.1 for day +39.
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$\begin{figure} \par\includegraphics[width=10cm]{10651f36.eps} \end{figure}$	Figure A.9: Spectropolarimetry of SN 2006X on day -7. Main line identifications are given in the upper panel. The red histogram traces the polarization along the dominant axys. Vertical dashed lines correspond to an expansion velocity of 19,000 km s^-1, while the dotted lines correspond to 14,000 km s^-1.
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$\begin{figure} \par\includegraphics[width=10cm]{10651f37.eps} \end{figure}$	Figure A.10: Same as Fig. A.9 for day -3. Vertical dashed lines correspond to a expansion velocity of 17,000 km s^-1, while the dotted lines correspond to 12,000 km s^-1.
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$\begin{figure} \par\includegraphics[width=10cm]{10651f38.eps} \end{figure}$	Figure A.11: Same as Fig. A.9 for day -1. Vertical dashed lines correspond to an expansion velocity of 16,000 km s^-1, while the dotted lines correspond to 11,000 km s^-1.
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$\begin{figure} \par\includegraphics[width=10cm]{10651f39.eps} \end{figure}$	Figure A.12: Same as Fig. A.9 for day +39. Vertical dotted lines correspond to a expansion velocity of 13,000 km s^-1.
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