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File:Asteroseismic HR diagram.svg

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Summary

Description
English: A Hertzsprung–Russell diagram, showing the luminosities and surface temperatures at which many classes of pulsating stars are found. Additional lines indicate where stars are found when they first fuse hydrogen into helium (zero-age main sequence, ZAMS), evolutionary tracks for stars of masses between 1 and 10 times that of the Sun, and the track along which a typical white dwarf of about 60% the Sun's mass cools.
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Source Own work
Author Warrickball

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Captions

A Hertzsprung–Russell diagram highlighting regions where many classes of pulsating star are found.

1 April 2023

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current11:22, 20 September 2023Thumbnail for version as of 11:22, 20 September 2023721 × 541 (94 KB)WarrickballUploaded own work with UploadWizard

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