Decoding the RVb Enigma of DF Cyg: Pulsations, Circumstellar Disks, and Post-RGB Evolution Revealed by Multi-Wavelength Observations

TL;DR

This study combines five decades of ground-based and recent space-based observations to analyze the pulsation, circumstellar environment, and evolutionary status of DF Cyg, revealing new pulsation harmonics and refining stellar parameters.

Contribution

It provides the first detailed analysis of DF Cyg using four years of Kepler and TESS data, uncovering new pulsation harmonics and improving understanding of its evolutionary phase.

Findings

Identified seven new integer harmonics of the fundamental pulsation frequency.

Detected approximately 35 frequencies related to variability mechanisms.

Confirmed stellar parameters consistent with Type II Cepheid relations.

Abstract

This investigation integrates five decades of ground-based photometric data from the AAVSO, AFOEV, ASAS, ASAS-SN, and SuperWASP surveys with recently acquired TESS observations, conducting a multi-wavelength and multi-phase photometric analysis to elucidate the complex nature of DF Cyg. For the first time, we analyze approximately four years of Kepler data alongside TESS observations. Furthermore, TESS observations obtained in 120-second cadence mode, constitute the highest-precision photometric dataset for DF Cyg to date. By isolating long-term trends in the TESS data, we quantified short-term variations in the fundamental pulsation frequency and its integer harmonics. The two alternating short-term cycles in the TESS light curve facilitated the unambiguous identification of seven previously undetected integer harmonics of the fundamental frequency in the power spectrum, providing critical new insights into the star's complex pulsation dynamics. A periodogram analysis of the combined ground- and space-based datasets revealed approximately 35 frequencies linked to both long- and short-term variability mechanisms. Stellar parameters derived from Gaia DR3 data specifically, luminosity and radius estimates based on Type II Cepheid PL and PR relations demonstrate consistency with values obtained through SED modeling. Complementary high-resolution spectroscopic analysis of DF Cyg yielded atmospheric parameters of Teff = 4781 K, logg = 1.74 dex, and [FeH] = -0.07 dex, further constraining physical characteristics of the star. This synthesis of multi-epoch, multi-instrument data advances the understanding of pulsational behavior and evolutionary status in RV Tauri systems. Our findings highlight DF Cyg as a critical benchmark for its class, as its characteristics bridge the gap between post-RGB systems in the Magellanic Clouds and higher-luminosity post-AGB stars.