PRODIGE -- Envelope to disk with NOEMA. VIII. Sulfur oxides trace a shock caused by a streamer in the inner envelope of a protostar

Recently, streamers have been observed causing shocks at the outer edge of protoplanetary disks. The study of sulfur-bearing species can help us to understand the physical and chemical changes caused by infalling streamers toward their landing positions. We study the physical properties traced by the emission of and SO toward the Class I protostar Per-emb 50, which is possibly related to the streamer infalling toward its disk. We present new NOrthern Extended Millimeter Array (NOEMA) A-array observations as part of the large program “Protostars and Disks: Global Evolution” (PRODIGE). We analyzed the morphology of and SO, and complement our interpretations with additional ̋tCO and CO data from the same program. We compared the and SO morphology with an infalling-rotating model. We applied Bayesian model selection to the brightest line to disentangle the different kinematic components traced by this molecule. We used local thermodynamic equilibrium (LTE) and non-LTE analyses to determine the temperature and density of the emission. There are two separate peaks of emission offset toward the southwest of Per-emb 50: one brighter (peak 1) at about 180 au from the protostar, and a weaker one (peak 2) at about 400 au. Peak 2 is blueshifted with respect to an infalling-rotating envelope. We propose that this peak is caused by the shock between the inner envelope and the streamer. Peak 1 is consistent with the expected envelope motion, and could thus be caused by shocks at the disk-envelope interface, but potential streamer influence cannot be neglected. Both peaks show abundance ratios consistent with a low-velocity shock (∼ 3-4 ̨ms) when compared with shock models. Streamers can affect the physical and chemical structure of both disks and envelopes, suggesting that streamers can play an important role in shaping both structures in the embedded stages of star formation.