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From the following article:

A runaway collision in a young star cluster as the origin of the brightest supernova

Simon F. Portegies Zwart & Edward P. J. van den Heuvel

Nature 450, 388-389(15 November 2007)

doi:10.1038/nature06276

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Figure 1

Mass of the collision runaway star as a function of cluster mass and its distance to the centre of NGC 1260.

Full size figure and legend (71K)
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