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Asteroseismology of the Red Giant Companions to Gaia BH2 and BH3

  • Authors: Daniel Hey, Yaguang Li, 亚光 李, J. M. Joel Ong, 加冕 王

Daniel Hey et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 5.

Power spectrum of BH3*. The red line is the power spectrum convolved with a Gaussian kernel of width 0.2 μHz, to highlight the absence of any significant signal. The blue vertical and horizontal lines correspond to the predicted power excess and power of the asteroseismic signal.

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