Occultation of the T Tauri Star RW Aurigae A by its Tidally Disrupted Disk
Joseph E. Rodriguez, Joshua Pepper, Keivan G. Stassun, Robert J., Siverd, Phillip Cargile, Thomas G. Beatty, B. Scott Gaudi

TL;DR
This study reports a deep, long-lasting dimming event of RW Aur A, attributed to a fragment of its tidally disrupted disk occulting the star, providing insights into the star's circumstellar environment post-interaction.
Contribution
The paper presents observational evidence linking a dimming event to a tidally disrupted disk fragment, offering new understanding of circumstellar disk dynamics after stellar fly-bys.
Findings
The dimming lasted approximately 180 days with a depth of ~2 magnitudes.
The occulter's velocity matches the relative velocity of the tidally disrupted arm.
The occulting feature is not part of the star's circumstellar disk.
Abstract
RW Aur A is a classical T Tauri star, believed to have undergone a reconfiguration of its circumstellar environment as a consequence of a recent fly-by of its stellar companion, RW Aur B. This interaction stripped away part of the circumstellar disk of RW Aur A, leaving a tidally disrupted arm and a short truncated circumstellar disk. We present photometric observations of the RW Aur system from the Kilodegree Extremely Little Telescope (KELT) survey showing a long and deep dimming that occurred from September 2010 until March 2011. The dimming has a depth of ~2 magnitudes, a duration of ~180 days and was confirmed by archival observations from American Association of Variable Star Observers (AAVSO). We suggest that this event is the result of a portion of the tidally disrupted disk occulting RW Aur A, specifically a fragment of the tidally disrupted arm. The calculated transverse…
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