2018 census of interstellar, circumstellar, extragalactic, protoplanetary disk, and exoplanetary molecules

BA McGuire - The Astrophysical Journal Supplement Series, 2018 - iopscience.iop.org
To date, 204 individual molecular species, comprised of 16 different elements, have been
detected in the interstellar and circumstellar medium by astronomical observations. These …

2021 census of interstellar, circumstellar, extragalactic, protoplanetary disk, and exoplanetary molecules

BA McGuire - The Astrophysical Journal Supplement Series, 2022 - iopscience.iop.org
To date, 241 individual molecular species, composed of 19 different elements, have been
detected in the interstellar and circumstellar medium by astronomical observations. These …

Rotational action spectroscopy of trapped molecular ions

O Asvany, S Schlemmer - Physical Chemistry Chemical Physics, 2021 - pubs.rsc.org
Rotational action spectroscopy is an experimental method in which rotational spectra of
molecules, typically in the microwave to sub-mm-wave domain of the electromagnetic …

[HTML][HTML] Laboratory spectroscopy techniques to enable observations of interstellar ion chemistry

BA McGuire, O Asvany, S Brünken… - Nature Reviews …, 2020 - nature.com
Molecular ions have long been considered key intermediates in the evolution of molecular
complexity in the interstellar medium. However, owing to their reactivity and transient nature …

The chemistry and spatial distribution of small hydrocarbons in UV-irradiated molecular clouds: the Orion Bar PDR

S Cuadrado, JR Goicoechea, P Pilleri… - Astronomy & …, 2015 - aanda.org
Context. Carbon chemistry plays a pivotal role in the interstellar medium (ISM) but even the
synthesis of the simplest hydrocarbons and how they relate to polycyclic aromatic …

Discovery of C5H+ and detection of C3H+ in TMC-1 with the QUIJOTE line survey

J Cernicharo, M Agúndez, C Cabezas… - Astronomy & …, 2022 - aanda.org
We report the discovery of the C 5 H+ cation toward TMC-1 with the QUIJOTE line survey.
Four lines from J= 7− 6 up to J= 10− 9 have been identified in perfect harmonic frequency …

The observed chemical structure of L1544

S Spezzano, P Caselli, L Bizzocchi… - Astronomy & …, 2017 - aanda.org
Context. Prior to star formation, pre-stellar cores accumulate matter towards the centre. As a
consequence, their central density increases while the temperature decreases …

LABORATORY ROTATIONAL SPECTRUM OF l–C3H+ AND CONFIRMATION OF ITS ASTRONOMICAL DETECTION

S Brünken, L Kluge, A Stoffels, O Asvany… - The Astrophysical …, 2014 - iopscience.iop.org
The rotational spectrum of l–C 3 H+ has been measured in the millimeter-wave band in a 4
K cryogenic ion trap apparatus employing a novel mass-selective action spectroscopy …

The interstellar chemistry of C3H and C3H2 isomers

JC Loison, M Agúndez, V Wakelam… - Monthly Notices of …, 2017 - academic.oup.com
We report the detection of linear and cyclic isomers of C3H and C3H2 towards various
starless cores and review the corresponding chemical pathways involving neutral (C3H x …

Gas-Phase Vibrational Spectroscopy of the Hydrocarbon Cations lC3H+, HC3H+, and cC3H2+: Structures, Isomers, and the Influence of Ne-Tagging

S Brünken, F Lipparini, A Stoffels… - The Journal of …, 2019 - ACS Publications
We report the first gas-phase vibrational spectra of the hydrocarbon ions C3H+ and C3H2+.
The ions were produced by electron impact ionization of allene. Vibrational spectra of the …