The Gaia-ESO Survey and CSI 2264: Substructures, disks, and sequential star formation in the young open cluster NGC 2264

L. Venuti; L. Prisinzano; G. G. Sacco; E. Flaccomio; R. Bonito; F. Damiani; G. Micela; M. G. Guarcello; S. Randich; J. R. Stauffer; A. M. Cody; R. D. Jeffries; S. H. P. Alencar; E. J. Alfaro; A. C. Lanzafame; E. Pancino; A. Bayo; G. Carraro; M. T. Costado; A. Frasca; P. Jofré; L. Morbidelli; S. G. Sousa; S. Zaggia

doi:10.1051/0004-6361/201731103

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Volume 609 (January 2018)

A&A, 609 (2018) A10

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Fig. 5

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Left panel: comparison between the A_V estimates derived for cluster members following methods 1. (y-axis) and 2. (x-axis) of Sect. 4.1. Right panel: comparison between the A_V estimates derived following methods 1. (y-axis) and 3. (x-axis) of Sect. 4.1. Each dot corresponds to an object; colors are scaled according to the objects’ T_eff, as shown on the side axes of the diagrams. The dashed lines trace the equality line on the diagrams.

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