Doppler images of II Pegasi for 2004-2010
Thomas Hackman, Maarit J. Mantere, Marjaana Lindborg, Ilya Ilyin, Oleg, Kochukhov, Nikolai Piskunov, Ilkka Tuominen

TL;DR
This study analyzes the long-term magnetic activity of II Pegasi from 2004 to 2010 using Doppler imaging, revealing a transition to a low-activity state with more randomly distributed spots compared to previous years.
Contribution
The paper provides new Doppler imaging maps of II Pegasi over 2004-2010, showing a shift from active longitude drift to a low-activity, more random spot distribution, indicating a possible activity cycle minimum.
Findings
Star's activity level decreased compared to 1994-2002.
No clear drift of active regions was observed during 2004-2010.
Star may be near a minimum of its activity cycle.
Abstract
Aims. We study the spot activity of II Peg during the years 2004-2010 to determine long- and short-term changes in the magnetic activity. In a previous study, we detected a persistent active longitude, as well as major changes in the spot configuration occurring on a timescale of shorter than a year. The main objective of this study is to determine whether the same phenomena persist in the star during these six years of spectroscopic monitoring. Methods. The observations were collected with the high-resolution SOFIN spectrograph at the Nordic Optical Telescope. The temperature maps were calculated using a Doppler imaging code based on Tikhonov regularization. Results. We present 12 new temperature maps that show spots distributed mainly over high and intermediate latitudes. In each image, 1-3 main active regions can be identified. The activity level of the star is clearly lower than…
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