TESS Observations of TX Col: Rapidly Varying Accretion Flow

Using the first long-term photometry from the Transiting Exoplanet Survey Satellite, we have carried out a detailed time-resolved timing analysis of an intermediate polar TX Col. The power spectra of almost 52 days of continuous time-series data reveal the orbital period of 5.691 +/- 0.006 hr, spin period of 1909.5 +/- 0.2 s, and beat period of 2105.76 +/- 0.25 s, which is consistent with the earlier results. We have also found the presence of quasi-periodic oscillations (QPOs) for a few days with a period of 5850-5950 s, which appears to be due to the beating of the Keplerian period with the spin period of the white dwarf. The continuous data allowed us to look thoroughly at the day-wise evolution of the system's accretion geometry. We report here that the TX Col changes its accretion mechanism even on a timescale of one day, confirming its variable disk-overflow accretion nature. For the majority of the time, it was found to be disk-overflow system with stream-fed dominance; however, pure disk-fed and pure stream-fed accretions cannot be ruled out during the observations.

Automated summary

By analyzing long-term photometry data, detailed periodic characteristics of the intermediate polar TX Col were studied. Changes in its accretion mechanism and the presence of quasi-periodic oscillations were observed over several days.