Prebiotic astrochemistry and the formation of molecules of astrobiological interest in interstellar clouds and protostellar disks

SA Sandford, M Nuevo, PP Bera, TJ Lee - Chemical reviews, 2020 - ACS Publications
Despite the generally hostile nature of the environments involved, chemistry does occur in
space. Molecules are seen in environments that span a wide range of physical and chemical …

Spitzer's perspective of polycyclic aromatic hydrocarbons in galaxies

A Li - Nature Astronomy, 2020 - nature.com
Polycyclic aromatic hydrocarbon (PAH) molecules are abundant and widespread throughout
the Universe, as revealed by their distinctive set of emission bands at 3.3, 6.2, 7.7, 8.6, 11.3 …

Detection of the aromatic molecule benzonitrile (c-C6H5CN) in the interstellar medium

BA McGuire, AM Burkhardt, S Kalenskii… - Science, 2018 - science.org
Polycyclic aromatic hydrocarbons and polycyclic aromatic nitrogen heterocycles are thought
to be widespread throughout the universe, because these classes of molecules are probably …

Interstellar polycyclic aromatic hydrocarbon molecules

AGGM Tielens - Annu. Rev. Astron. Astrophys., 2008 - annualreviews.org
Large polycyclic aromatic hydrocarbon (PAH) molecules carry the infrared (IR) emission
features that dominate the spectra of most galactic and extragalactic sources. This review …

The molecular universe

A Tielens - Reviews of Modern Physics, 2013 - APS
Molecular absorption and emission bands dominate the visible, infrared, and submillimeter
spectra of most objects with associated gas. These observations reveal a surprisingly rich …

Aromatic hexazine [N6]4− anion featured in the complex structure of the high-pressure potassium nitrogen compound K9N56

D Laniel, F Trybel, Y Yin, T Fedotenko… - Nature …, 2023 - nature.com
The recent high-pressure synthesis of pentazolates and the subsequent stabilization of the
aromatic [N5]− anion at atmospheric pressure have had an immense impact on nitrogen …

The NASA Ames PAH IR spectroscopic database: The laboratory spectra

AL Mattioda, DM Hudgins, C Boersma… - The Astrophysical …, 2020 - iopscience.iop.org
The astronomical emission features, formerly known as the unidentified infrared bands, are
now commonly ascribed to polycyclic aromatic hydrocarbons (PAHs). The laboratory …

The NASA Ames PAH IR spectroscopic database: Computational version 3.00 with updated content and the introduction of multiple scaling factors

CW Bauschlicher, A Ricca, C Boersma… - The Astrophysical …, 2018 - iopscience.iop.org
Abstract Version 3.00 of the library of computed spectra in the NASA Ames PAH IR
Spectroscopic Database (PAHdb) is described. Version 3.00 introduces the use of multiple …

The diffuse interstellar bands: A major problem in astronomical spectroscopy

PJ Sarre - Journal of Molecular Spectroscopy, 2006 - Elsevier
A critical review of the very long-standing problem of the diffuse interstellar bands is
presented with emphasis on spectroscopic aspects of observational, modelling and …

Coupling photochemistry with haze formation in Titan's atmosphere, part I: Model description

PP Lavvas, A Coustenis, IM Vardavas - Planetary and Space Science, 2008 - Elsevier
We introduce a new 1D coupled Radiative/Convective-Photochemical-Microphysical model
for a planetary atmosphere and apply it to Titan. The model incorporates detailed radiation …