Nova-Like Cataclysmic Variable TT Ari: QPO Behaviour Coming Back From Positive Superhumps
Y. Kim, I.L. Andronov, S.M.Cha, L.L.Chinarova J.-N. Yoon

TL;DR
This study analyzes the variability and QPO behavior of TT Ari, a nova-like cataclysmic variable, during its transition from positive to negative superhump states, revealing consistent QPO periods and significant short-term variations.
Contribution
It provides detailed observational analysis of TT Ari's QPOs and superhump states, highlighting the stability of QPO periods and variability across different activity phases.
Findings
QPOs have a mean period of 21.6 minutes with semi-amplitude of 36 mmag.
The QPO period does not show secular decrease over time.
Significant night-to-night variations in QPO period and amplitude.
Abstract
We study the variability of the nova-like cataclysmic variable TT Ari, on time-scales of between minutes and months. The observations in the filter R were obtained at the 40-cm telescope of the Chungbuk National University (Korea). TT Ari was in the "negative superhump" state after its return from the "positive superhump" state, which lasted 8 years. The ephemeris for 12 best pronounced minima is where numbers in digits are errors in units of the last digit. The phases of minima may reach 0.2, indicating non-eclipse nature of these minima. The quasi-periodic oscillations (QPO) are present with a mean "period" of 21.6 min and mean semi-amplitude of 36 mmag. This value is consistent with the range 15-25 minutes reported for previous "negative superhump" states and does not support the hypothesis of secular decrease of the QPO period. Either…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Particle Accelerators and Free-Electron Lasers · Pulsars and Gravitational Waves Research
