Showing 1–18 of 18 results
/ Date/ Name
Sep 8, 2025Understanding JWST water spectra: what can thermochemical models tell us about the (cold) water in protoplanetary disks?Aug 6, 2025A transition from H$_2$O to C$_2$H$_2$ dominated spectra with decreasing stellar luminosityAug 4, 2025MINDS. Young binary systems with JWST/MIRI: Variable water-rich primaries and extended emissionJul 15, 2025Chemical transformation of CO in evolving protoplanetary discs across stellar masses: a route to C-rich inner regionsMay 21, 2025MINDS. Water reservoirs of compact planet-forming dust disk: A diversity of H$_2$O distributionsApr 15, 2025MINDS: The very low-mass star and brown dwarf sample -- Hidden water in carbon-dominated protoplanetary disksDec 17, 2024MINDS. JWST-MIRI reveals a peculiar CO$_2$-rich chemistry in the drift-dominated disk CX TauDec 2, 2024CO2-rich protoplanetary discs as a probe of dust radial drift & trappingAug 1, 2024Photoevaporation of protoplanetary discs with PLUTO+PRIZMO I. Lower X-ray-driven mass-loss rates due to enhanced coolingMar 14, 2024Modeling JWST MIRI-MRS Observations of T Cha: Mid-IR Noble Gas Emission Tracing a Dense Disk WindJan 11, 2024Correlation between accretion rate and free-free emission in protoplanetary disks -- A multi-wavelength analysis of central mm/cm emission in transition disksOct 4, 2023FRIED v2. A new grid of mass loss rates for externally irradiated protoplanetary discsApr 20, 2022The importance of X-ray frequency in driving photoevaporative windsMar 8, 2022The evolution of protoplanetary discs in star formation and feedback simulationsJun 9, 2021The general applicability of self-similar solutions for thermal disc windsDec 16, 2020Proplyds in the Flame Nebula NGC 2024Aug 17, 2020A dusty origin for the correlation between protoplanetary disc accretion rates and dust massesDec 12, 2019The evolution of dust in discs influenced by external photoevaporation