Optical microflares in LS I +61 303 and the search for their multiwavelength counterpart

TL;DR

This study uses high-precision optical and gamma-ray data to discover small-amplitude microflares in the binary system LS I +61 303, providing new insights into its optical behavior and potential multiwavelength counterparts.

Contribution

It presents the first detection of optical microflares in LS I +61 303 using space-based photometry, expanding understanding of stellar gamma-ray sources.

Findings

Detected optical microflares with amplitudes below 0.01 magnitude

Proposed multiple scenarios for the origin of the microflares

Utilized archival data from TESS and Fermi observatories

Abstract

Stellar sources of gamma rays are one of the front lines in modern astrophysics whose understanding can benefit from observational tools not originally designed for their study. We take advantage of the high precision photometric capabilities of present-day space facilities to obtain a new perspective on the optical behavior of the X-ray and gamma-ray binary LS I +61 303. Previously unknown phenomena whose effects manifest with amplitudes below 0.01 magnitude can now be clearly observed and studied. Our work is mainly based on the analysis of optical and gamma-ray archival data and uses the tools recommended by the different collaborations that provide these valuable observational resources (in particular, the TESS and Fermi orbiting observatories). In addition, complementary ground-based optical spectroscopy has also been conducted. We report the discovery of small-amplitude optical flares on timescales of a day in the LS I +61 303 light curve. Different alternative scenarios to explain their origin are tentatively proposed.