S. Rodriguez

collaborators

2 papers

astro-ph.EP2026

An unidentified absorption feature at 5.11 $I^¼$ m on the surface of Titan and Pluto from JWST spectroscopy

B. BÃ©zard, E. Lellouch, M. Camarca +14

Titan possesses a thick N $_{2}$ -CH $_{4}$ atmosphere that makes it difficult to study its surface spectroscopically. The chemical composition of the solid surface of Titan thus remains…

astro-ph.GA2025

PDRs4All XIX. The 6 to 9 $I^¼$ m region as a probe of PAH charge and size in the Orion Bar

Baria Khan, Samuel A. Daza Rodriguez, Els Peeters +24

Infrared emission from polycyclic aromatic hydrocarbons (PAHs) play a major role in determining the charge balance of their host environments that include photo-dissociation region…

An unidentified absorption feature at 5.11 I^¼m on the surface of Titan and Pluto from JWST spectroscopy

PDRs4All XIX. The 6 to 9 I^¼m region as a probe of PAH charge and size in the Orion Bar

An unidentified absorption feature at 5.11 $I^¼$ m on the surface of Titan and Pluto from JWST spectroscopy

PDRs4All XIX. The 6 to 9 $I^¼$ m region as a probe of PAH charge and size in the Orion Bar