[MRAS] Benzene has been detected across a range of astrophysical environments, though the primary mechanism underpinning its formation has not yet been constrained and the extreme conditions of the interstellar […]
benzene
Aromatic Rings In The Central Molecular Zone: Benzonitrile
In recent years, several aromatic molecules (benzene-based rings) have been detected in the cold molecular cloud TMC-1, with its CN-derivative, benzonitrile (c-C6H5CN), also identified in other nearby cold sources.
Functionalization Of Benzene Ices by Atomic Oxygen
Small aromatic molecules, including functionalized derivatives of benzene, are known to be present throughout the different stages of star and planet formation. In particular, oxygen-bearing monosubstituted aromatics, likely including phenol, […]
Hybrid Approach Predicts A Lower Binding Energy For Benzene On Water Ice
In this paper we provide a highly accurate value for the binding energy of benzene to proton-ordered crystalline water ice (XIh), as a model for interstellar ices.
Abundant Hydrocarbons in the Disk Around a Very-low-mass Star
Very low-mass stars (those <0.3 solar masses) host orbiting terrestrial planets more frequently than other types of stars, but the compositions of those planets are largely unknown.
Planet-forming Disks Around Very Low-mass Stars Are Different
Planets form in disks of gas and dust, orbiting young stars. The MIRI Mid-INfrared Disk Survey (MINDS), led by Thomas Henning from the Max Planck Institute for Astronomy (MPIA) in […]
A Pole-to-Pole Map Of Hydrocarbons In Saturn’s Upper Stratosphere And Mesosphere
We analyze data from the final two years of the Cassini mission to retrieve the distributions of methane, ethane, acetylene, ethylene, and benzene in Saturn’s upper stratosphere and mesosphere from […]
Astronomers Spot Benzene In A Planet-forming Disk Around Star J160532 For The First Time
An international team of astronomers including several Dutch researchers has observed the benzene molecule (C6H6) in a planet-forming disk around a young star for the first time.
Polyaromatic Hydrocarbons with an Imperfect Aromatic System as Catalysts of Interstellar H2 Formation
Although H2 is the simplest and the most abundant molecule in the Universe, its formation in the interstellar medium, especially in the photodissociation regions is far from being fully understood.
