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The 2020 Eclipse of R Aquarii in the Near-infrared: Mid-eclipse Observations of Disk Distress

  • Authors: Kenneth H. Hinkle, Sean Brittain, Francis C. Fekel, Thomas Lebzelter, Adwin Boogert

Kenneth H. Hinkle et al 2022 The Astrophysical Journal 937 .

  • Provider: AAS Journals

Caption: Figure 6.

Radial velocity of the peak emission of 12C16O lines as a function of the lower-level excitation energy of the transition. Filled symbols are from 2020 August, open symbols are from 2020 September. The dashed line is a linear fit to the data. The systemic velocity of the binary is −24.9 ± 0.2 km s−1 (Gromadzki & Mikołajewska 2009) with the Mira velocity ∼−24 km s−1 and the WD velocity ∼−27 km s−1 on the dates of the observations.

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