activity
20172026
most citedThe chemistry of cosmic dust analogues from C, C, and CH in C-rich circumstellar envelopes

45 citations · 84 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2026

The Significant Role of Hydrogen in the Formation of Silicon Carbide in Evolved Stars

Guillermo Tajuelo-Castilla, Gonzalo Santoro, Lidia Martínez +13

Cosmic dust is mainly formed in the atmospheres of evolved stars. In carbon rich stars, amorphous carbon along with silicon carbide are the main constituents of dust grains yet the…

astro-ph.IM2020★ 7 cited

INFRA-ICE: an ultra-high vacuum experimental station for laboratory astrochemistry

Gonzalo Santoro, Jesús. M. Sobrado, Guillermo Tajuelo-Castilla +7

Laboratory astrochemistry aims at simulating in the laboratory some of the chemical and physical processes that operate in different regions of the Universe. Amongst the diverse as…

astro-ph.GA2020★ 18 cited

Silicon and hydrogen chemistry under laboratory conditions mimicking the atmosphere of evolved stars

Mario Accolla, Gonzalo Santoro, Pablo Merino +10

Silicon is present in interstellar dust grains, meteorites and asteroids, and to date thirteen silicon-bearing molecules have been detected in the gas-phase towards late-type stars…

astro-ph.GA2020★ 45 cited

The chemistry of cosmic dust analogues from C, C, and CH in C-rich circumstellar envelopes

Gonzalo Santoro, Lidia Martínez, Koen Lauwaet +13

Interstellar carbonaceous dust is mainly formed in the innermost regions of circumstellar envelopes around carbon-rich asymptotic giant branch (AGB) stars. In these highly chemical…

astro-ph.IM2017★ 14 cited

Using radio astronomical receivers for molecular spectroscopic characterization in astrochemical laboratory simulations: A proof of concept

I. Tanarro, B. Alemán, P. de Vicente +26

We present a proof of concept on the coupling of radio astronomical receivers and spectrometers with chemical reactorsand the performances of the resulting setup for spectroscopy a…