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arXiv · 2608.10388

An Optically Motivated Gamma-ray Study of Fermi-LAT Novae

Owen K. Henry·Timothy A. D. Paglione·David Zurek·Joshua Tan
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Abstract

High-energy (GeV) gamma-ray emission from nova eruptions was a surprise detection by the Fermi-LAT in 2010. Since then, it has been suggested that the gamma-rays from these systems are generated in collisionless non-relativistic shocks. In this theory, the observed correlation between optical and gamma-ray nova lightcurves naturally arises if a portion of the optical luminosity is reprocessed shock power. In this work, we investigate this scenario by analyzing Fermi-LAT-detected novae in varied time bins and then correlating the bin size that maximizes the nova's significance (tgam) with the nova's optical eruption data. Furthermore, we investigate whether there is a common optical decay across the sources' measured tgam values in the population. We find that across our population, a nova's $t_3$ (the time it takes the nova V band brightness to decay 3 magnitudes) appears to be the favored analysis bin that optimizes the Fermi-LAT detection significance, although there is significant spread. Additionally, we report V679 Car, a source previously noted as a marginally detected gamma-ray nova, as a $>5 σ$ detection in this work. We perform cross-correlation analysis of gamma-ray and optical lightcurves.

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Owen K. Henry, Timothy A. D. Paglione, David Zurek, Joshua Tan. 2026-08-11. An Optically Motivated Gamma-ray Study of Fermi-LAT Novae. https://arxiv.org/abs/2608.10388

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