File:Asteroseismic HR diagram.svg
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Size of this PNG preview of this SVG file: 769 × 577 pixels. Other resolutions: 320 × 240 pixels | 640 × 480 pixels | 1,024 × 768 pixels | 1,280 × 960 pixels | 2,560 × 1,921 pixels.
Original file (SVG file, nominally 769 × 577 pixels, file size: 94 KB)
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. |
| Date | |
| Source | Own work |
| Author | Warrickball |
Licensing
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File history
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 20:52, 5 September 2025 | | 769 × 577 (94 KB) | wikimediacommons>Warrickball | swap DBV and DAV labels to correct positions |
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