Figure 5 from ABUNDANCES, STELLAR PARAMETERS, AND SPECTRA FROM THE SDSS-III/APOGEE SURVEY

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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 5.

Internal elemental abundance calibrations. Plots show deviations of individual elements relative to the cluster means as a function of temperature; these have been defined to be zero at 4500 K. Different symbols are for different clusters, as noted in lower right. Lines shows the adopted temperature calibrations. Carbon and nitrogen are not shown because we cannot assume homogeneous abundances within clusters.

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