The astrodust+ PAH model: A unified description of the extinction, emission, and polarization from dust in the diffuse interstellar medium
BS Hensley, BT Draine - The Astrophysical Journal, 2023 - iopscience.iop.org
We present a new model of interstellar dust in which large grains are a single composite
material," astrodust," and nanoparticle-sized grains come in distinct varieties including …
material," astrodust," and nanoparticle-sized grains come in distinct varieties including …
Observational constraints on the physical properties of interstellar dust in the post-Planck era
BS Hensley, BT Draine - The Astrophysical Journal, 2021 - iopscience.iop.org
We present a synthesis of the astronomical observations constraining the wavelength-
dependent extinction, emission, and polarization from interstellar dust from UV to microwave …
dependent extinction, emission, and polarization from interstellar dust from UV to microwave …
A Vision for the Future of Astrochemistry in the Interstellar Medium by 2050
RC Fortenberry - ACS Physical Chemistry Au, 2023 - ACS Publications
By 2050, many, but not nearly all, unattributed astronomical spectral features will be
conclusively linked to molecular carriers (as opposed to nearly none today in the visible and …
conclusively linked to molecular carriers (as opposed to nearly none today in the visible and …
Multifacets of Fullerene–Metal Clusters: From Fundamental to Application
J Xu, YK Li, E Janssens, GL Hou - Accounts of Chemical Research, 2024 - ACS Publications
Conspectus Buckminsterfullerene, C60, was discovered through a prominent mass peak
containing 60 atoms produced from laser vaporization of graphite, driven by Kroto's interest …
containing 60 atoms produced from laser vaporization of graphite, driven by Kroto's interest …
Prevalence of non-aromatic carbonaceous molecules in the inner regions of circumstellar envelopes
Evolved stars are foundries of chemical complexity, gas and dust that provide the building
blocks of planets and life, and dust nucleation first occurs in their photosphere. The …
blocks of planets and life, and dust nucleation first occurs in their photosphere. The …
Towards a reliable prediction of the infrared spectra of cosmic fullerenes and their derivatives in the JWST era
ABSTRACT Fullerenes, including C60, C70, and C60+, are widespread in space through
their characteristic infrared vibrational features (C60+ also reveals its presence in the …
their characteristic infrared vibrational features (C60+ also reveals its presence in the …
[HTML][HTML] C60+ as a diffuse interstellar band carrier; a spectroscopic story in 6 acts
In 2019 it was exactly 100 years ago that the first two DIBs, diffuse interstellar bands, were
discovered by Mary Lea Heger. Today some 500+ DIBs are known. In numerous …
discovered by Mary Lea Heger. Today some 500+ DIBs are known. In numerous …
Electronic spectroscopy of monocyclic carbon ring cations for astrochemical consideration
J Rademacher, ES Reedy… - The Journal of Physical …, 2022 - ACS Publications
Gas phase electronic spectra of pure carbon cations generated by laser vaporization of
graphite in a supersonic jet and cooled to below 10 K and tagged with helium atoms in a …
graphite in a supersonic jet and cooled to below 10 K and tagged with helium atoms in a …
CRIRES high-resolution near-infrared spectroscopy of diffuse interstellar band profiles-Detection of 12 new DIBs in the YJ band and the introduction of a combined …
A Ebenbichler, A Postel, N Przybilla, A Seifahrt… - Astronomy & …, 2022 - aanda.org
Aims. A high spectral resolution investigation of diffuse interstellar bands (DIBs) in the near-
infrared (YJ band) is conducted to test new methods, to confirm and improve existing …
infrared (YJ band) is conducted to test new methods, to confirm and improve existing …
Buckyball-metal complexes as potential carriers of astronomical unidentified infrared emission bands
Efforts over 40 yr still leave the source of astronomical infrared emission bands largely
unidentified. Here, we report the first laboratory infrared (6–25 μm) spectra of gas-phase …
unidentified. Here, we report the first laboratory infrared (6–25 μm) spectra of gas-phase …