activity
20132026
most citedDetection of the Ammonium Ion in Space

62 citations · 187 across the 10 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

5 papers · 1 filter

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.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.GA2013★ 21 cited

Improved determination of the 1(0)-0(0) rotational frequency of NH3D+ from the high resolution spectrum of the v4 infrared band

J. L. Doménech, M. Cueto, V. J. Herrero +4

The high resolution spectrum of the v4 band of NH3D+ has been measured by difference frequency IR laser spectroscopy in a multipass hollow cathode discharge cell. From the set of m…

astro-ph.GA2013★ 62 cited

Detection of the Ammonium Ion in Space

J. Cernicharo, B. Tercero, A. Fuente +9

We report on the detection of a narrow feature at 262816.73 MHz towards Orion and the cold prestellar core B1-bS, that we attribute to the 1(0)-0(0) line of the deuterated Ammonium…