Organic molecules in the interstellar medium, comets, and meteorites: a voyage from dark clouds to the early Earth

P Ehrenfreund, SB Charnley - Annual Review of Astronomy and …, 2000 - annualreviews.org
▪ Abstract Our understanding of the evolution of organic molecules, and their voyage from
molecular clouds to the early solar system and Earth, has changed dramatically …

Experimentally tracing the key steps in the origin of life: The aromatic world

P Ehrenfreund, S Rasmussen, J Cleaves, L Chen - Astrobiology, 2006 - liebertpub.com
Life is generally believed to emerge on Earth, to be at least functionally similar to life as we
know it today, and to be much simpler than modern life. Although minimal life is notoriously …

Laboratory confirmation of C60+ as the carrier of two diffuse interstellar bands

EK Campbell, M Holz, D Gerlich, JP Maier - Nature, 2015 - nature.com
The diffuse interstellar bands are absorption lines seen towards reddened stars. None of the
molecules responsible for these bands have been conclusively identified. Two bands at …

[图书][B] Dust in the galactic environment

DCB Whittet - 2018 - taylorfrancis.com
Dust is a ubiquitous feature of the cosmos, impinging directly or indirectly on most fields of
modern astronomy and astrophysics. Dust in the Galactic Environment, Second Edition …

Confirming interstellar C using the Hubble Space Telescope

MA Cordiner, H Linnartz, NLJ Cox, J Cami… - arXiv preprint arXiv …, 2019 - arxiv.org
Recent advances in laboratory spectroscopy lead to the claim of ionized
Buckminsterfullerene (C60+) as the carrier of two diffuse interstellar bands (DIBs) in the near …

Ubiquitous aromatic carbon chemistry at the earliest stages of star formation

AM Burkhardt, RA Loomis, CN Shingledecker… - Nature …, 2021 - nature.com
Abstract Benzonitrile (c-C6H5CN, where 'c'indicates a cyclic structure), a polar proxy for
benzene (c-C6H6), has the potential to serve as a highly convenient radio probe for …

Identification of more interstellar bands

GAH Walker, DA Bohlender, JP Maier… - The Astrophysical …, 2015 - iopscience.iop.org
Based on gas-phase laboratory spectra at 6 K, Campbell et al. confirmed that the diffuse
interstellar bands (DIBs) at 9632.7 and 9577.5 Å are due to absorption by the fullerene ion …

Formation of polycyclic aromatic hydrocarbons and carbonaceous solids in gas-phase condensation experiments

C Jäger, F Huisken, H Mutschke, IL Jansa… - The Astrophysical …, 2009 - iopscience.iop.org
Carbonaceous grains represent a major component of cosmic dust. In order to understand
their formation pathways, they have been prepared in the laboratory by gas-phase …

Gas phase absorption spectroscopy of and in a cryogenic ion trap: comparison with astronomical measurements

EK Campbell, M Holz, JP Maier, D Gerlich… - The Astrophysical …, 2016 - iopscience.iop.org
Recent low-temperature laboratory measurements and astronomical observations have
proved that the fullerene cation ${{\rm {C}}} _ {60}^{+} $ is responsible for four diffuse …

Interstellar fullerene compounds and diffuse interstellar bands

A Omont - Astronomy & Astrophysics, 2016 - aanda.org
Recently, the presence of fullerenes in the interstellar medium (ISM) has been confirmed
and new findings suggest that these fullerenes may possibly form from polycyclic aromatic …