File:Remnants of single massive stars.svg

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English: Remnants of massive single stars as a function of initial mass and initial content of elements heavier than Helium (metallicity)
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Source Own work based on A. Heger, C. L. Fryer, S. E. Woosley, N. Langer, D. H. Hartmann: How massive single stars end their life. The Astrophysical Journal, 591:288–300, 2003 July 1
Author Fulvio314
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Date/TimeThumbnailDimensionsUserComment
current17:08, 16 April 2020Thumbnail for version as of 17:08, 16 April 2020512 × 315 (5 KB)Jarvisa (talk | contribs)Simplified SVG source
10:21, 28 November 2013Thumbnail for version as of 10:21, 28 November 2013512 × 315 (366 KB)Fulvio314 (talk | contribs)=={{int:filedesc}}== {{Information |description={{en|1=Remnants of massive single stars as a function of initial mass and initial content of elements heavier than Helium (metallicity)}} |date=2013-11-28 11:00:00 |source={{own}} based on [http://iopscie...

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