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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 2.

Power spectrum of RGB17. The gray curve represents the power density spectrum, and purple is the smoothed spectrum. The power excess of the solar-like oscillations is between the two yellow lines, while the red line is the linear background fit within this range. The ﹩{\nu }_{{\rm{\max }}}﹩ estimated by the pyMON code is indicated as a vertical dashed purple line.

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