File:Red dwarfs2.png

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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/TimeThumbnailDimensionsUserComment
current16:03, 19 February 2020Thumbnail for version as of 16:03, 19 February 2020940 × 731 (348 KB)Meli thev (talk | contribs)User created page with UploadWizard

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