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ABUNDANCES, STELLAR PARAMETERS, AND SPECTRA FROM THE SDSS-III/APOGEE SURVEY

  • Authors: Jon A. Holtzman, Matthew Shetrone , Jennifer A. Johnson, Carlos Allende Prieto, Friedrich Anders, Brett Andrews, Timothy C. Beers, Dmitry Bizyaev, Michael R. Blanton, Jo Bovy, Ricardo Carrera, S. Drew Chojnowski, Katia Cunha, Daniel J. Eisenstein, Diane Feuillet, Peter M. Frinchaboy, Jessica Galbraith-Frew, Ana E. García Pérez, D. A. García-Hernández, Sten Hasselquist, Michael R. Hayden, Fred R. Hearty, Inese Ivans, Steven R. Majewski, Sarah Martell, Szabolcs Meszaros, Demitri Muna, David Nidever, Duy Cuong Nguyen, Robert W. O'Connell, Kaike Pan, Marc Pinsonneault, Annie C. Robin, Ricardo P. Schiavon, Neville Shane, Jennifer Sobeck, Verne V. Smith, Nicholas Troup, David H. Weinberg, John C. Wilson, W. M. Wood-Vasey, Olga Zamora, and Gail Zasowski

2015 The Astronomical Journal 150 148.

  • Provider: AAS Journals

Caption: Figure 16.

Persistence comparison for CNO abundances for stars with ﹩H\gt 11.﹩ Left panel has stars with all observations outside of persistence region, while right panel has stars with all observations inside of persistence region. Points are color-coded by temperature; black points have empirical uncertainties greater than 0.1 dex.

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