Results 111 to 120 of about 8,526 (198)
Astrochemistry: Synthesis and Modelling [PDF]
We discuss models that astrochemists have developed to study the chemical composition of the interstellar medium. These models aim at computing the evolution of the chemical composition of a mixture of gas and dust under as- trophysical conditions. These conditions, as well as the geometry and the physical dynamics, have to be adapted to the objects ...
arxiv
PREBIOTIC ASTROCHEMISTRY IN THE "THz-GAP" [PDF]
Fundamental biological molecules such as amino acids and sugars have been discovered in meteorites, but none of these species have yet been definitively detected in the interstellar medium (ISM). While both the number of detected interstellar molecules and their chemical complexity continue to increase, understanding of the processes leading to their ...
openaire +2 more sources
Infrared (IR) spectral features of interstellar and solar system ices have been attributed to solid organic and inorganic compounds for over 50 yr, but in many cases the laboratory IR data needed to fully quantify such work have never been published ...
Reggie L. Hudson+2 more
doaj +1 more source
The van der Waals dispersion coefficients of a set of polycyclic aromatic hydrocarbons, ranging in size from the single-cycle benzene to circumovalene (C66H20), are calculated with a real-time propagation approach to time-dependent density functional ...
Alberto Castro+9 more
core +3 more sources
Single‐Step Control of Liquid–Liquid Crystalline Phase Separation by Depletion Gradients
Different sizes of nanoparticles with concentration gradients control the liquid–liquid crystalline phase separation (LLCPS) speed and induce different morphologies of tactoids with positional order. Nanoparticles can be templated by LLCPS via size selectivity effects inside and on the surface of tactoids, enabling unprecedented spatial ...
Dongdong Lin+5 more
wiley +1 more source
Astrochemistry in an Ion Storage Ring
Storage ring studies of low energy electron collisions with molecular ions have been carried out for dissociative recombination (DR) of fluorine-bearing molecules. Here we report on work aiming to improve the understanding of astrochemistry involving HF, a possible spectroscopic tracer of interstellar H2.
Steffen Novotny+22 more
openaire +4 more sources
Detection of the simplest sugar, glycolaldehyde, in a solar-type protostar with ALMA
Glycolaldehyde (HCOCH2OH) is the simplest sugar and an important intermediate in the path toward forming more complex biologically relevant molecules. In this paper we present the first detection of 13 transitions of glycolaldehyde around a solar-type ...
Beltrán+17 more
core +1 more source
The UMIST Database for Astrochemistry 2022
Context. Detailed astrochemical models are a key component to interpret the observations of interstellar and circumstellar molecules since they allow important physical properties of the gas and its evolutionary history to be deduced. Aims. We update one of the most widely used astrochemical databases to reflect advances in experimental and theoretical
T. J. Millar+3 more
openaire +5 more sources
A full dimensional Potential Energy Surface (PES) of the CO + N2 system has been generated by extending an approach already reported in the literature and applied to N2-N2 (Cappelletti et al., 2008), CO2-CO2 (Bartolomei et al., 2012), and CO2-N2 ...
Andrea Lombardi+7 more
doaj +1 more source
Water Vapor in the Inner 25 AU of a Young Disk around a Low-Mass Protostar
Water is one of the key molecules in the physical and chemical evolution of star- and planet-forming regions. We here report the first spatially resolved observation of thermal emission of (an isotopologue of) water with the Plateau de Bure ...
Jorgensen, Jes K.+1 more
core +1 more source