Search for the third component in the PZ Mon system — a synchronous binary star of RS CVn type
Abstract
In 2015-2017, new measurements of the radial velocities were performed for the PZ Mon system. An orbital period of the second component is improved and amounts now to P = 34.123 & plusmn; 0.002d. Analysis of residual velocities did not show a presence of the third component in the system.
- Publication:
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A.A. Boyarchuk Memorial Conference
- Pub Date:
- May 2018
- DOI:
- Bibcode:
- 2018abmc.conf...62P