Spotted Surface Structure of the Active Giant PZ Mon


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Abstract

Based on our photometric observations in 2015–2016 and archival photometric data for the active red giant PZ Mon, we have found the main characteristics of the stellar surface: the unspotted surface temperature Teff = 4730 K, the spot temperature Ts = 3500 K, and the relative spot area from 30 to 40%. The best agreement with the observations has been achieved in our three-spot model including a cool polar spot with a temperature of ~3500 K as well as large and small warm spots with a temperature of ~4500 K. The stable polar spot is responsible for the long-period brightness variations. Its presence is confirmed by an analysis of the TiO 7054 Å molecular band. The small-amplitude 34-day variability is attributable to the warm spots located on the side of the secondary component, which determine the relatively stable active longitude.

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About the authors

Yu. V. Pakhomov

Institute of Astronomy

Author for correspondence.
Email: pakhomov@inasan.ru
Russian Federation, Pyatnitskaya ul. 48, Moscow, 109017

K. A. Antonyuk

Crimean Astrophysical Observatory

Email: pakhomov@inasan.ru
Russian Federation, Nauchny, Crimea, 298409

N. I. Bondar’

Crimean Astrophysical Observatory

Email: pakhomov@inasan.ru
Russian Federation, Nauchny, Crimea, 298409

N. V. Pit’

Crimean Astrophysical Observatory

Email: pakhomov@inasan.ru
Russian Federation, Nauchny, Crimea, 298409

I. V. Reva

Fesenkov Astrophysical Institute

Email: pakhomov@inasan.ru
Kazakhstan, Almaty

A. V. Kusakin

Fesenkov Astrophysical Institute

Email: pakhomov@inasan.ru
Kazakhstan, Almaty

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