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A Possible Changing Systemic Velocity for CV Serpentis: Further Evidence of a Third Body in the Dust-making Wolf–Rayet Binary?

  • Authors: Em Biegler, Noel D. Richardson, André-Nicolas Chené, Emma P. Lieb, William Punches

Em Biegler et al 2026 Research Notes of the AAS 10 .

  • Provider: AAS Journals

Caption: Figure 1.

Here we plot the systemic velocity of CV Ser both for the WR star (C III 5696, black circles) and the O star (He II 5411, blue asterisks) compared to the average date for each calendar year’s observation time. We include the times of the individual observations for both GHOST and MAROON-X at the top of the plot. The points for the two lines measured are separated by 15 d of time for clarity.

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