L. Waters

collaborators

2 papers

astro-ph.SR2025

MINDS. Cha HÎ± 1, a brown dwarf with a hydrocarbon-rich disk

MarÃa Morales-CalderÃ³n, Hyerin Jang, Aditya M. Arabhavi +23

Context. Recent JWST observations have shown that brown dwarfs (BD) are chemically rich, offering valuable insights into giant planet formation. Aims. As part of the MIRI mid-INfra…

astro-ph.EP2025

A transition from H $_{2}$ O to C $_{2}$ H $_{2}$ dominated spectra with decreasing stellar luminosity

Sierra L. Grant, Milou Temmink, Ewine F. van Dishoeck +19

The chemical composition of the inner regions of disks around young stars will determine the properties of planets forming there. Many disk physical processes drive the chemical ev…

MINDS. Cha HÎ± 1, a brown dwarf with a hydrocarbon-rich disk

A transition from H2​O to C2​H2​ dominated spectra with decreasing stellar luminosity

A transition from H $_{2}$ O to C $_{2}$ H $_{2}$ dominated spectra with decreasing stellar luminosity