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The Mass–Activity Relationships in M and K Dwarfs. I. Stellar Parameters of Our Sample of M and K Dwarfs

  • Authors: Éric R. Houdebine, D. J. Mullan, J. G. Doyle, Geoffroy de La Vieuville, C. J. Butler, and F. Paletou

2019 The Astronomical Journal 158 56.

  • Provider: AAS Journals

Caption: Figure 2.

Comparison between two sets of values of Teff: (i) taken from the literature and (ii) derived from the (RI)C/Teff correlations that have been derived by M15 and B12. Continuous line: the correlation that would exist if there was an exact one-to-one correspondence between the two sets of Teff. Dashed line: the best-fit correlation when the data are smoothed by a Gaussian of FWHM 30 K. Note that there exists a good overall agreement between the smoothed data and the expectations of a one-to-one correspondence.

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