2026-06-08T04:38:24Zhttps://docta.ucm.es/rest/oai/request

oai:docta.ucm.es:20.500.14352/49932024-07-12T13:27:11Zcom_20.500.14352_14col_20.500.14352_15

Vallejo Chavarino, Juan C. Gómez De Castro, Ana Inés 2023-06-16T14:25:22Z 2023-06-16T14:25:22Z 2021-09-11 0035-8711 10.1093/mnras/stab2581 https://hdl.handle.net/20.500.14352/4993 https://doi.org/10.1093/mnras/stab2581 Protoplanetary discs are complex dynamical systems where several processes may lead to the formation of ring-like structures and planets. These discs are flared following a profile where the vertical scale height increases with radius. In this work, we investigate the role of this disc flaring geometry on the formation of rings and holes. We combine a flattening law change with X-ray and FUV photoevaporative winds. We have used a semi-analytical 1D viscous α approach, presenting the evolution of the disc mass and mass rate in a grid of representative systems. Our results show that changing the profile of the flared disc may favour the formation of ring-like features resembling those observed in real systems at the proper evolutionary times, with proper disc masses and accretion rate values. However, these features seem to be short-lived and further enhancements are still needed for better matching all the features seen in real systems. eng open access Formation of ring-like structures in flared U-discs with X-ray/FUV photoevaporation journal article