Results 61 to 70 of about 1,176,456 (219)

Chemical Kinetics of 2‐, 4‐, and 2,4‐Seleno‐Uracils at Low Temperatures: Tautomerizations and Rotamerizations on Inert Matrices

open access: yesInternational Journal of Chemical Kinetics, Volume 58, Issue 10, Page 881-889, October 2026.
ABSTRACT In the interstellar medium, chemical reactions proceed under conditions vastly different to those on Earth; these include extremely low temperatures and densities and take place in the gas phase and on water–ice grains. Understanding the energetics and more importantly the kinetics of such reactions is of relevance to the consequences on how ...
Judith Wurmel, John M. Simmie
wiley   +1 more source

Synthesis of Molecules in Interstellar Clouds & Star Formation [PDF]

open access: yes, 1981
237-240Study of the formation and destruction processes of interstellar molecules may throw certain light on interstellar medium. Formation and destruction processes of some interstellar molecules are proposed on the basis of laboratory data.
Ghosh, K K, Ghosh, S N
core  

Interstellar Ices: A Factory of the Origin-of-Life Molecules [PDF]

open access: yes
Interstellar-ice chemistry paves the way for disclosing the mystery of the origin of life: amino acids and other prebiotic molecules are formed in ...
Puzzarini C., Alessandrini S.
core   +1 more source

From Flybys to Sample Return: A Review of Space Probes and Robotic Sampling Technologies for Small Bodies

open access: yesJournal of Field Robotics, Volume 43, Issue 7, Page 4475-4514, October 2026.
ABSTRACT As a crucial puzzle piece of deep space exploration, exploring small bodies can provide significant scientific insights and valuable mineral resources. Unlike missions to the Moon and Mars, small‐body missions pose distinct technical challenges, including communication delays, weak gravity, and uncertain environments. This paper reviews a full
Xin Zhang   +3 more
wiley   +1 more source

Protonated interstellar ions of diatomic molecules : quantum-mechanical predictions

open access: yes, 2004
The present role of Quantum Chemistry in the field of interstellar molecules is illustrated by structure and reactivity studies concerning the (CS + H) +, (SiO + H)+, (SiS + H ...
G. Berthier
core   +1 more source

H2 Ortho–Para Spin Conversion on Inhomogeneous Grain Surfaces. II. Impact of the Rotational Energy Difference between Adsorbed Ortho-H2 and Para-H2 and Implication for Deuterium Fractionation Chemistry

open access: yesThe Astrophysical Journal
We investigate how the H _2 ortho-to-para ratio (OPR) and deuterium fractionation in star-forming regions are affected by nuclear spin conversion (NSC) on dust grains. Particular focus is placed on the rotational energy difference between ortho-H _2 (o-H
Kenji Furuya   +4 more
doaj   +1 more source

Proximity Proteomics Maps Candidate Cellular Uptake Pathways for Cell‐Derived Nanovesicles

open access: yesSmall Methods, Volume 10, Issue 19, 7 October 2026.
TurboID‐based dual‐sided proteomics compares mechanically generated cell‐derived nanovesicles with naturally secreted small extracellular vesicles. Vesicle proteomes define candidate interaction signatures, while recipient‐cell proximity labelling identifies exposure‐associated proteins.
Eisuke Kanao   +8 more
wiley   +1 more source

Lifetimes of Certain Interstellar Organic Molecules [PDF]

open access: yes, 1981
78-79Lifetimes of some organic molecules such as H2CO, H2CS, HCOOH, CH3NH2, CH3OH and CH3CHO in interstella, space against photodissociation and chemical reactions in the gas phase have been calculated.
Ghosh, K K, Ghosh, S N
core  

SYSTEMATIC THEORETICAL STUDY ON THE INTERSTELLAR CARBON CHAIN MOLECULES

open access: yes, 2016
In an effort to further our interest in understanding the basic chemistry of interstellar molecules, here we carry out an extensive investigation of the stabilities of interstellar carbon chains; C-n, H2Cn, HCnN and CnX (X = N, O, Si, S, H, P, H-, N ...
Gorai, Prasanta   +6 more
core   +1 more source

Interstellar Molecules - The Optical Region [PDF]

open access: yesHighlights of Astronomy, 1971
Considerable attention has recently been given to the observation of interstellar molecules by radio methods. Interstellar molecules have also been given a boost because of excitation by the 3K black body radiation field (to use a convenient description).
openaire   +1 more source

Home - About - Disclaimer - Privacy