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Integrated Mass Loss for Very Metal-poor Stars: Asterosesimic Red Giant Masses of K2 Globular Cluster NGC 5897

  • Authors: Csilla Kalup, László Molnár, Madeline Howell, Attila Bódi, András Pál

Csilla Kalup et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure A2.

Calculated corrected color excesses (C*) based on M. Riello et al. (2021), in order to evaluate the Gaia DR3 GBP and GRP photometry against G. The dark blue points are stars from panel (c) of Figure A1. Overmarks in light pink and dark red represent RGB and EAGB stars, respectively. Dashed blue lines correspond to the 7σ scatter, while the solid red curves are for 10σ, see more information in Appendix A. This figure confirms the nature and positions of our sample stars, with a particular regard for EAGB10, EAGB11, and RGB27.

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