We report here a new result extracted from the Fermi Large Area Telescope observation of the classical nova ASASSN-16ma that exhibits coherent gamma-ray pulsations at 544.84(7) seconds during its outburst in 2016. Considering the number of independent trials, the significance of the evidence is 4.0 sigma, equivalent to a false alarm probability of 5.9e-5. The periodicity was steady during the 4 days of its appearance, indicating its origin as the spinning signal of the white dwarf. Given that the optical and gamma-ray light curves of some shock-powered gamma-ray novae have been recently shown closely correlated to each other, the gamma-ray pulsation phenomenon likely implies an existence of the associated optical pulsations, which would provide detailed ephemerides for these extreme white dwarf binaries for further investigations in the near future.
@article{arxiv.2201.03218,
title = {Evidence for Gamma-Ray Pulsations from the Classical Nova ASASSN-16ma},
author = {Kwan-Lok Li},
journal= {arXiv preprint arXiv:2201.03218},
year = {2022}
}
Comments
7 pages, including 4 figures. Accepted for publication in ApJL