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From the following article:

The binary progenitor of Tycho Brahe's 1572 supernova

Pilar Ruiz-Lapuente, Fernando Comeron, Javier Méndez, Ramon Canal, Stephen J. Smartt, Alexei V. Filippenko, Robert L. Kurucz, Ryan Chornock, Ryan J. Foley, Vallery Stanishev and Rodrigo Ibata

Nature 431, 1069-1072(28 October 2004)

doi:10.1038/nature03006

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Figure 1 - Unfortunately we are unable to provide accessible alternative text for this. If you require assistance to access this image, or to obtain a text description, please contact npg@nature.com

Figure 1

Positions and proper motions of stars.

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Figure 2

The SN 1572 field and radial velocity of the stars.

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Figure 3

Model fits to observed spectra.

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Table 1

Characteristics of the supernova companion candidates

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