Turnitin
降AI改写
早检测系统
早降重系统
Turnitin-UK版
万方检测-期刊版
维普编辑部版
Grammarly检测
Paperpass检测
checkpass检测
PaperYY检测
Thermal desorption of interstellar ices: A review on the controlling parameters and their implications from snowlines to chemical complexity
The evolution of star-forming regions and their thermal balance are strongly influenced by
their chemical composition, which, in turn, is determined by the physicochemical processes …
their chemical composition, which, in turn, is determined by the physicochemical processes …
Spiers memorial lecture: Astrochemistry at high resolution
Astrochemistry is the science that studies the chemistry in the Universe, namely the
combination of two fields: astronomy and chemistry. It started about fifty years ago and it has …
combination of two fields: astronomy and chemistry. It started about fifty years ago and it has …
Quantum mechanical simulations of the radical–radical chemistry on icy surfaces
The formation of the interstellar complex organic molecules (iCOMs) is a hot topic in
astrochemistry. One of the main paradigms trying to reproduce the observations postulates …
astrochemistry. One of the main paradigms trying to reproduce the observations postulates …
Theoretical distribution of the ammonia binding energy at interstellar icy grains: A new computational framework
The binding energies (BE) of molecules on the interstellar grains are crucial in the chemical
evolution of the interstellar medium (ISM). Both temperature-programmed desorption (TPD) …
evolution of the interstellar medium (ISM). Both temperature-programmed desorption (TPD) …
Binding energy evaluation platform: A database of quantum chemical binding energy distributions for the astrochemical community
The quality of astrochemical models is highly dependent on reliable binding energy (BE)
values that consider the morphological and energetic variety of binding sites on the surface …
values that consider the morphological and energetic variety of binding sites on the surface …
Binding energies of interstellar relevant S-bearing species on water ice mantles: a quantum mechanical investigation
Binding energies (BEs) are one of the most important parameters for astrochemical
modeling determining, because they govern whether a species stays in the gas phase or is …
modeling determining, because they govern whether a species stays in the gas phase or is …
Theoretical Water Binding Energy Distribution and Snowline in Protoplanetary Disks
Water is one of the most important and abundant molecules in star-forming regions. In
protoplanetary disks, where planets and comets form, H 2 O is in a gas or solid form …
protoplanetary disks, where planets and comets form, H 2 O is in a gas or solid form …
Computer Generated Realistic Interstellar Icy Grain Models: Physicochemical Properties and Interaction with NH3
Interstellar grains are composed by a rocky core (usually amorphous silicates) covered by
an icy mantle, the most abundant molecule being H2O followed by CO, CO2, NH3, and also …
an icy mantle, the most abundant molecule being H2O followed by CO, CO2, NH3, and also …
In-depth exploration of catalytic sites on amorphous solid water: I. The astrosynthesis of aminomethanol
Chemical processes taking place on ice-grain mantles are pivotal to the complex chemistry
of interstellar environments. In this study, we conducted a comprehensive analysis of the …
of interstellar environments. In this study, we conducted a comprehensive analysis of the …
Assessing realistic binding energies of some essential interstellar radicals with amorphous solid water-A fully quantum chemical approach
In the absence of laboratory data, state-of-the-art quantum chemical approaches can
provide estimates of the binding energy (BE) of interstellar species with grains. Without BE …
provide estimates of the binding energy (BE) of interstellar species with grains. Without BE …