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The R-process Alliance: The Peculiar Chemical Abundance Pattern of RAVE J183013.5−455510

  • Authors: Vinicius M. Placco, Rafael M. Santucci, Zhen Yuan, Mohammad K. Mardini, Erika M. Holmbeck, Xilu Wang, Rebecca Surman, Terese T. Hansen, Ian U. Roederer, Timothy C. Beers, Arthur Choplin, Alexander P. Ji, Rana Ezzeddine, Anna Frebel, Charli M. Sakari, Devin D. Whitten, and Joseph Zepeda

2020 The Astrophysical Journal 897 78.

  • Provider: AAS Journals

Caption: Figure 2.

Spectral syntheses for the determination of the abundances of carbon (upper panel), nitrogen (middle panel), and oxygen (lower right panel). The top panel of each plot shows the best-fit syntheses (blue lines) and uncertainties (shaded regions) compared to the observed spectra (points). Also shown are syntheses after removing all the contributions from specific elements (gray lines). The bottom panels show the residuals between the observed spectra and the syntheses. The lower left panel shows the determination of the 12C/13C ratio (see text for details).

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