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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 1.

CMD of NGC 5897 based on Johnson B and V photometry by P. B. Stetson et al. (2019). The colored points represent the initial RG sample we searched for solar-like oscillations. The 21 dark red dots correspond to EAGB stars, while the 49 light pink points show RGB stars.

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