Electron–molecule collision calculations using the R-matrix method

J Tennyson - Physics Reports, 2010 - Elsevier
The R-matrix method is an embedding procedure which is based on the division of space
into an inner region where the physics is complicated and an outer region for which greatly …

BASECOL2012: A collisional database repository and web service within the Virtual Atomic and Molecular Data Centre (VAMDC)

ML Dubernet, MH Alexander, YA Ba… - Astronomy & …, 2013 - aanda.org
The BASECOL2012 database is a repository of collisional data and a web service within the
Virtual Atomic and Molecular Data Centre (VAMDC, http://www. vamdc. eu). It contains rate …

Detection of a Noble Gas Molecular Ion, 36ArH+, in the Crab Nebula

MJ Barlow, BM Swinyard, PJ Owen, J Cernicharo… - Science, 2013 - science.org
Noble gas molecules have not hitherto been detected in space. From spectra obtained with
the Herschel Space Observatory, we report the detection of emission in the 617.5-and …

BASECOL2023 scientific content

ML Dubernet, C Boursier, O Denis-Alpizar… - Astronomy & …, 2024 - aanda.org
Context. The global context of making numerous data produced by researchers available
requires collecting and organising the data, assigning meaningful metadata, and presenting …

Comparative study of CH+ and SH+ absorption lines observed towards distant star-forming regions

B Godard, E Falgarone, M Gerin, DC Lis… - Astronomy & …, 2012 - aanda.org
Aims. The HIFI instrument onboard Herschel has allowed high spectral resolution and
sensitive observations of ground-state transitions of three molecular ions: the methylidyne …

Excited OH+, H2O+, and H3O+ in NGC 4418 and Arp 220

E González-Alfonso, J Fischer, S Bruderer… - Astronomy & …, 2013 - aanda.org
We report on Herschel/PACS observations of absorption lines of OH+, H 2 O+ and H 3 O+ in
NGC 4418 and Arp 220. Excited lines of OH+ and H 2 O+ with E lower of at least 285 and …

The chemistry of ions in the Orion Bar I.–CH+, SH+, and CF+-The effect of high electron density and vibrationally excited H2 in a warm PDR surface

Z Nagy, FFS Van der Tak, V Ossenkopf, M Gerin… - Astronomy & …, 2013 - aanda.org
Context. The abundances of interstellar CH+ and SH+ are not well understood as their most
likely formation channels are highly endothermic. Several mechanisms have been proposed …

Laser probing of the rotational cooling of molecular ions by electron collisions

Á Kálosi, M Grieser, R von Hahn, U Hechtfischer… - Physical Review Letters, 2022 - APS
We present state-selected measurements of rotational cooling and excitation rates of CH+
molecular ions by inelastic electron collisions. The experiments are carried out at a …

Electron-impact rotational excitation of linear molecular ions

A Faure, J Tennyson - Monthly Notices of the Royal …, 2001 - academic.oup.com
Molecular R-matrix calculations are performed to give rotational excitation rates for electron
collisions with linear molecular ions. Results are presented for CO+, HCO+, NO+ and H2+ …

A complete model of CH+ rotational excitation including radiative and chemical pumping processes

B Godard, J Cernicharo - Astronomy & Astrophysics, 2013 - aanda.org
Aims. Excitation of far-infrared and submillimetric molecular lines may originate from
nonreactive collisions, chemical formation, or far infrared, near-infrared, and optical …