Updated photometry and orbital period analysis for the polar \objectname{am herculis} on the upper edge of the period gap
Zhibin Dai, Shengbang Qian, Linjia Li

TL;DR
This study presents updated photometric data and analysis of AM Herculis, revealing a 12-15 year periodic variation in its orbital period and discussing potential mechanisms behind this modulation.
Contribution
The paper provides the first comprehensive long-term optical light curve analysis and updated O-C diagram for AM Herculis, identifying a significant periodic orbital variation.
Findings
Detected a 12-15 year sine-like variation in the O-C diagram.
Discovered 16 new primary minima and 7 low-state transient events.
Discussed possible mechanisms for the orbital period modulation.
Abstract
Twenty-one new optical light curves, including five curves obtained in 2009 and sixteen curves detected from the AAVSO International Database spanning from 1977 to 2011, demonstrate 16 new primary minimum light times in the high state. Furthermore, seven newly found low-state transient events from 2006 to 2009 were discovered, consisting of five Gaussian-shaped events and two events with an exponential form with decay timescales of 0.005 days; these timescales are one order of magnitude shorter than those of previous X-ray flare events. In the state transition, two special events were detected: a "disrupted event" with an amplitude of 2 mag and a duration of 72 minutes and continuing R-band twin events larger than all known R-band flares detected in M-type red dwarfs. All 45 available high-state data points spanning over 35 yr were used to construct an updated O-C…
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