Publications (4)
Predicting the detectability of sulphur-bearing molecules in the solid phase with simulated spectra of JWST instruments
A. Taillard, R. MartÃn-Doménech, H. Carrascosa +7
To date, gas phase observations of sulphur in dense interstellar environments have only constrained the molecular carriers of 1% of its predicted cosmic abundance. An additional 5%…
Characterization of carbon dioxide on Ganymede and Europa supported by experiments: Effects of temperature, porosity, and mixing with water
L. Schiltz, B. Escribano, G. M. Muñoz Caro +8
The surfaces of icy moons are primarily composed of water ice that can be mixed with other compounds, such as carbon dioxide. The carbon dioxide (CO stretching fundamental ban…
UV-photoprocessing of acetic acid (CH3COOH)-bearing interstellar ice analogs
C. del Burgo Olivares, H. Carrascosa, B. Escribano +2
Acetic acid (CH3COOH) was detected in the gas toward interstellar clouds, hot cores, protostars and comets. Its formation in ice mantles was proposed and acetic acid awaits detecti…
Physical properties of methanol (CHOH) ice as a function of temperature: Density, infrared band strengths, and crystallization
H. Carrascosa, M. Ã. Satorre, B. Escribano +2
The presence of methanol among the common ice components in interstellar clouds and protostellar envelopes has been confirmed by the James Webb Space Telescope. Methanol is often d…