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Astronomy & Astrophysics 606 A109 (2017)
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A theoretical study of the dissociative recombination of SH+ with electrons through the 2Π states of SH

D. O. Kashinski, D. Talbi, A. P. Hickman, O. E. Di Nallo, F. Colboc, K. Chakrabarti, I. F. Schneider and J. Zs. Mezei
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Rovibrationally resolved photodissociation of SH+

E C McMillan, G Shen, J F McCann, B M McLaughlin and P C Stancil
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https://doi.org/10.1088/0953-4075/49/8/084001

Rotational Spectrum, Conformational Composition, Intramolecular Hydrogen Bonding, and Quantum Chemical Calculations of Mercaptoacetonitrile (HSCH2C≡N), a Compound of Potential Astrochemical Interest

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Electron-impact excitation of diatomic hydride cations – I. HeH+, CH+, ArH+

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The Cologne Database for Molecular Spectroscopy, CDMS, in the Virtual Atomic and Molecular Data Centre, VAMDC

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https://doi.org/10.1016/j.jms.2016.03.005

Quantum and quasi-classical calculations for the S+ + H2(v,j) → SH+(v′,j′) + H reactive collisions

Alexandre Zanchet, Octavio Roncero and Niyazi Bulut
Physical Chemistry Chemical Physics 18 (16) 11391 (2016)
https://doi.org/10.1039/C6CP00604C

Radiative charge transfer in cold and ultracold sulphur atoms colliding with protons

G Shen, P C Stancil, J G Wang, J F McCann and B M McLaughlin
Journal of Physics B: Atomic, Molecular and Optical Physics 48 (10) 105203 (2015)
https://doi.org/10.1088/0953-4075/48/10/105203

Using block diagonalization to determine dissociating autoionizing states: Application to N2H, and the outlook for SH

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A new study of an old sink of sulphur in hot molecular cores: the sulphur residue

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Magnetic Fields in Diffuse Media

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SUBMILLIMETER/THz ROTATIONAL SPECTROSCOPY OF SH+(${X}^{3}{{\rm{\Sigma }}}^{-}$): THE COMPLETEN= $1\leftarrow 0$ TRANSITION

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https://doi.org/10.1088/0004-637X/814/2/119

An ATCA survey of Sagittarius B2 at 7 mm: chemical complexity meets broad-band interferometry

Joanna F. Corby, Paul A. Jones, Maria R. Cunningham, et al.
Monthly Notices of the Royal Astronomical Society 452 (4) 3969 (2015)
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Ubiquitous argonium (ArH+) in the diffuse interstellar medium: A molecular tracer of almost purely atomic gas

P. Schilke, D. A. Neufeld, H. S. P. Müller, et al.
Astronomy & Astrophysics 566 A29 (2014)
https://doi.org/10.1051/0004-6361/201423727

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13 (2014)
https://doi.org/10.1002/9783527653133.ch2

Revised spectroscopic parameters of SH+from ALMA and IRAM 30 m observations

Holger S. P. Müller, Javier R. Goicoechea, José Cernicharo, et al.
Astronomy & Astrophysics 569 L5 (2014)
https://doi.org/10.1051/0004-6361/201424756

Herschel/HIFI Discoveryof a Far-Infrared DIB Analog

H. S. P. Müller, P. Schilke, M. Gerin, et al.
Proceedings of the International Astronomical Union 9 (S297) 197 (2013)
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CO(6−5) and [C i](2−1) pointed observations of five protoplanetary disks: Warm gas in HD 142527

S. Casassus, A. Hales, I. de Gregorio, et al.
Astronomy & Astrophysics 553 A64 (2013)
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Interstellar Water Chemistry: From Laboratory to Observations

Ewine F. van Dishoeck, Eric Herbst and David A. Neufeld
Chemical Reviews 113 (12) 9043 (2013)
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Complex organic molecules in the interstellar medium: IRAM 30 m line survey of Sagittarius B2(N) and (M)

A. Belloche, H. S. P. Müller, K. M. Menten, P. Schilke and C. Comito
Astronomy & Astrophysics 559 A47 (2013)
https://doi.org/10.1051/0004-6361/201321096

LABORATORY MEASUREMENTS AND TENTATIVE ASTRONOMICAL IDENTIFICATION OF H2NCO+

H. Gupta, C. A. Gottlieb, V. Lattanzi, J. C. Pearson and M. C. McCarthy
The Astrophysical Journal 778 (1) L1 (2013)
https://doi.org/10.1088/2041-8205/778/1/L1

SULFUR CHEMISTRY IN THE INTERSTELLAR MEDIUM: THE EFFECT OF VIBRATIONAL EXCITATION OF H2IN THE REACTION S++H2→SH++H

Alexandre Zanchet, Marcelino Agúndez, Victor J. Herrero, Alfredo Aguado and Octavio Roncero
The Astronomical Journal 146 (5) 125 (2013)
https://doi.org/10.1088/0004-6256/146/5/125

Ortho/Para Ratio of H2O+ Toward Sagittarius B2(M) Revisited

Peter Schilke, Dariusz C. Lis, Edwin A. Bergin, Ronan Higgins and Claudia Comito
The Journal of Physical Chemistry A 117 (39) 9766 (2013)
https://doi.org/10.1021/jp312364c

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

B. Godard, E. Falgarone, M. Gerin, et al.
Astronomy & Astrophysics 540 A87 (2012)
https://doi.org/10.1051/0004-6361/201117664

The impact of recent advances in laboratory astrophysics on our understanding of the cosmos

D W Savin, N S Brickhouse, J J Cowan, et al.
Reports on Progress in Physics 75 (3) 036901 (2012)
https://doi.org/10.1088/0034-4885/75/3/036901

Using deuterated H 3 + and other molecular species to understand the formation of stars and planets

F. F. S. van der Tak
Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 370 (1978) 5186 (2012)
https://doi.org/10.1098/rsta.2012.0026

Accurate theoretical study of PSq (q = 0,+1,−1) in the gas phase

Saida Ben Yaghlane, Joseph S. Francisco and Majdi Hochlaf
The Journal of Chemical Physics 136 (24) (2012)
https://doi.org/10.1063/1.4730303

Molecular line survey of the high-mass star-forming region NGC 6334I withHerschel/HIFI and the Submillimeter Array

A. Zernickel, P. Schilke, A. Schmiedeke, et al.
Astronomy & Astrophysics 546 A87 (2012)
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