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Summary
| Description |
English: The young star cluster NGC 2264, with a large number of T Tauri stars contracting towards the main sequence. The solid line represents the main sequence, while the two lines above that are the 10^6.5 yr (upper) and 10^6.7 yr (lower) isochrones. |
| Date | |
| Source | 1961-2011: Fifty years of Hayashi tracks (http://proceedings.aip.org/resource/2/apcpcs/1480/1/22_1) |
| Author | D.G. Turner |
Licensing
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This work is ineligible for copyright and therefore in the public domain because it consists entirely of information that is common property and contains no original authorship. |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 06:14, 7 May 2013 | | 422 × 547 (79 KB) | Bowlhover | User created page with UploadWizard |
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