Figure 7 from A Spectropolarimetric View on the Nature of the Peculiar Type I SN 2005hk

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A Spectropolarimetric View on the Nature of the Peculiar Type I SN 2005hk

Authors: Justyn R. Maund, J. Craig Wheeler, Lifan Wang, Dietrich Baade, Alejandro Clocchiatti, Ferdinando Patat, Peter Höflich, Jason Quinn, and Paula Zelaya

MAUND et al. 2010 The Astrophysical Journal 722 1162.

Provider: AAS Journals

Caption: Figure 7.

Spectropolarimetry of SN 2005hk on 2005 November 9, projected onto the dominant axis ( P _d ) and the orthogonal axis ( P _o ). The data have been binned to 30 Å for clarity and have been corrected for the ISP component. The weighted average of the ISP, rotated onto the dominant and orthogonal axes, is indicated by the heavy gray lines.

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