Can angular momentum loss cause the period change of NN Ser?
Wen-Cong Chen

TL;DR
This paper investigates whether angular momentum loss via a circumbinary disk can explain the observed period decrease in NN Ser, concluding that a third body is a more plausible explanation due to implausible required wind loss rates.
Contribution
The study proposes a circumbinary disk mechanism for angular momentum loss in NN Ser, but finds it unlikely, supporting the third body hypothesis instead.
Findings
Circumbinary disk can theoretically extract angular momentum from NN Ser.
High wind loss rates and disk feeding fractions are required, which are considered unrealistic.
A third body is a more plausible cause for the period change.
Abstract
NN Ser is a non mass-transferring pre-cataclysmic variable containing a white dwarf with a mass of and an M dwarf secondary star with a mass of . Based on the data detected by the high-speed CCD camera ULTRACAM, it was observed that the orbital period of NN Ser is decreasing, which may be caused by a genuine angular momentum loss or the presence of a third body. However, neither gravitational radiation and magnetic braking can ideally account for the period change of NN Ser. In this Letter, we attempt to examine a feasible mechanism which can drain the angular momentum from NN Ser. We propose that a fossil circumbinary disk (CB disk) around the binary may have been established at the end of the common envelope phase, and the tidal torques caused by the gravitational interaction between the disk and the binary can efficiently extract the orbital…
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