File:PMS evolution tracks.png

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English: Isochrones and evolutionary tracks for pre-main-sequence stars. The curves labeled in years are isochrones at the given ages. In other words, stars 1 x 105 years old lie along the curve labeled 1 x 105, and similarly for the other 3 isochrones. The darker curves, cutting across the isochrones, are evolutionary tracks. At the leftmost side, the tracks are labeled with the mass of the star (in solar masses) that they represent. A star of that mass follows its evolutionary track from 1 x 105 years, shortly after its birth, to 1 x 108 years, when it is on the main sequence.
Date
Source Francesco Palla, 1961–2011: Fifty years of Hayashi tracks, AIP Conf. Proc. 1480, pp. 22-29; doi:10.1063/1.4754323
Author Francesco Palla

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Date/TimeThumbnailDimensionsUserComment
current06:14, 7 May 2013Thumbnail for version as of 06:14, 7 May 2013467 × 477 (35 KB)BowlhoverUser created page with UploadWizard
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