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Summary
| Description |
English: The figure above, constructed using stars up to 100 parsecs (326 light years) from Earth identified by the Gaia spacecraft, shows the position of the red dwarf LHS 1678 in the Hertzsprung–Russell diagram. This star is located in a small gap in the diagram. This gap, which can be more accurately described as a star deficit, is associated with a transition from partially convective interiors to fully convective interiors in red dwarfs. |
| Date | |
| Source | https://iopscience.iop.org/article/10.3847/1538-3881/ac32e3/pdf |
| Author | Michele L. Silverstein et al. |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 13:36, 17 May 2024 | | 720 × 720 (309 KB) | 21.Andromedae | Expand |
| 15:17, 16 May 2024 |  | 711 × 717 (357 KB) | 21.Andromedae | Uploaded a work by Michele L. Silverstein et al. from https://iopscience.iop.org/article/10.3847/1538-3881/ac32e3/pdf with UploadWizard |
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