Impact of accretion variability on the CO emission of a disk around a very low-mass star with JWST
Context: Very low-mass stars (M_⋆<0.2M_⊙) are known to host a larger fraction of terrestrial planets compared to higher mass stars. Studying the structure of their protoplanetary disk is therefore crucial to understanding the formation of Earth-like planets. Aims: In this work, we aim to characterize the innermost regi...