# Superorbital modulation at GeV energies in the gamma-ray binary LS I +61 303

## TL;DR

This study analyzes 8 years of Fermi-LAT data on LS I +61 303, revealing superorbital phase shifts in gamma-ray emission likely caused by a rotating elliptical circumstellar disk around the Be star.

## Contribution

It provides the first detailed analysis linking superorbital gamma-ray modulation to a rotating elliptical circumstellar disk in LS I +61 303.

## Key findings

- Detected a significant dip around periastron in superorbital light curves.
- Observed phase shifts in superorbital modulation fitted with sinusoidal functions.
- Proposed that the disk's elliptical shape and rotation cause the observed phase shifts.

## Abstract

We report the results from our analysis of 8 years of the data for the gamma-ray binary LS I +61 303, obtained with the Large Area Telescope onboard the Fermi Gamma-Ray Space Telescope. We find a significant dip around the binary's periastron in the superorbital light curves, and by fitting the light curves with a sinusoidal function, clear phase shifts are obtained. The superorbital modulation seen in the binary has been long known and different scenarios have been proposed. Based on our results, we suggest that the circumstellar disk around the Be companion of this binary has an elliptical shape and the major axis of the disk rotates at the superorbital period of 1667 days. As a result, the density of the ambient material around the compact star of the binary changes along the binary orbit over the superorbital period, causing the phase shifts in the modulation, and around periastron, the compact star probably enters the disk, causing the appearance of the dip. Numerical simulations may be conducted in order to study the detailed physical processes and verify our suggestion.