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Summary
| Description |
English: M-dwarfs go from partly convective to fully convective and this is seen in the Hertzsprung–Russell diagram (Jao et al. 2018). To create this diagram I used ESA's Gaia Archive and the following selection method: G-mag<20, plx>15, astrometric_sigma5d_max<0.5 The stars plotted here are therefore closer than 217 light-years (67 parsec). |
| Date | |
| Source | ESA's Gaia Archive + Own work |
| Author | Meli thev |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 16:03, 19 February 2020 | | 940 × 731 (348 KB) | Meli thev | User created page with UploadWizard |
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