An explanation of the missing flux from Boyajian's mysterious star

TL;DR

This paper proposes that the missing flux in Boyajian's star's dimming events can be explained by the star's own convective processes, challenging external obscuration hypotheses and offering new insights into stellar magnetoconvection.

Contribution

It introduces a novel explanation for the missing flux in Boyajian's star based on stellar convection, expanding the understanding of its dimming phenomena.

Findings

Convective stellar models can account for the missing flux.

Explains asymmetry in dimming time profiles.

Accounts for long-term dimming trends.

Abstract

A previously unremarked star in the constellation Cygnus has,in the past year,become known as the most mysterious star in our Galaxy.Boyajian's star exhibits puzzling episodes of sporadic deep dimming discovered in photometry with the Kepler Mission. Proposed explanations have focused on its obscuration by colliding exoplanets, exocomets, and even intervention of alien intelligence. These hypotheses have considered only phenomena external to the star because the radiative flux missing in the dimmings was believed to exceed the star's storage capacity.We point out that modeling variations in solar luminosity indicates that convective stars can store the required fluxes. It also suggests explanations for a reported time profile asymmetry of the short,deep dimmings and for a slower,decadal scale dimming reported from archival and Kepler photometry. Our findings favor a broader range of explanations of Boyajian's star, that may produce new insights into stellar magnetoconvection.