The Recurrent Nova U Scorpii from the 2010.1 to 2022.4 Eruptions; the Missed Eruption of 2016.78 +- 0.10 and the Critical Complex Period Changes
Bradley E. Schaefer

TL;DR
This study analyzes multiple eruptions of the recurrent nova U Scorpii from 2010 to 2022, revealing complex period changes likely caused by asymmetric shell ejection and magnetic braking, and constraining a missed eruption in 2016.
Contribution
It provides detailed measurements of orbital period changes across eruptions, proposing a novel explanation involving asymmetric shell ejection and identifying a previously missed eruption in 2016.
Findings
Significant orbital period increase after 2010 eruption.
Large, variable period change attributed to magnetic braking.
Constrained the missed 2016 eruption to a specific 75-day interval.
Abstract
U Sco is a recurrent nova with eleven observed eruptions, most recently in 2010.1 and 2022.4. I report on my program (running since 1989) of measuring eclipse times and brightnesses of U Sco in quiescence, from 2010 to 2022. The orbital period suddenly increased by +22.4 +- 1.0 parts-per-million across the 2010.1 eruption. This period change is greater than the near-zero period change (+3.9 +- 6.1 parts-per-million) across the 1999.2 eruption. This period change cannot come from any of the usual mechanisms, whereas the one remaining possibility is that the period changes are dominated by the little-known mechanism of the nova ejecting asymmetric shells. From 2010.1 to 2016.78, the O-C curve showed a steady period change that was large, with P-dot equal (-21.0 +- 3.2)X 10^-9. This is greatly higher than the steady period changes in the two previous inter-eruption intervals (-3.2 +- 1.9…
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