Results 121 to 130 of about 37,732 (195)
The interstellar medium (ISM) is all but empty. To date, more than 300 molecules have already been discovered. Because of the extremely low temperature, the gas-phase chemistry is dominated by barrierless exothermic reactions of radicals and ions ...
Tobe Vorsselmans, Erik C. Neyts
doaj +1 more source
Formation and Processing of Interstellar Dust.
openaire +2 more sources
Direct Samples of Interstellar and Interplanetary Material with IMAP. [PDF]
Szalay JR +21 more
europepmc +1 more source
Chemistry in Extreme Environments: The Mystery of Molecular Complexity in Space. [PDF]
Puzzarini C, Alessandrini S.
europepmc +1 more source
Atom Addition Formation of Thionylimide (HNSO) on Interstellar Dust Grains: Chemical Routes Requiring Oxygen and Nitrogen Atom Surface Diffusion. [PDF]
Del Valle JC +6 more
europepmc +1 more source
Multiscale Perspectives on Solid-Phase Astrochemistry: Laboratory, Computation, and Open Questions. [PDF]
Dickers MD +3 more
europepmc +1 more source
Molecular clouds (MCs) in space are the birthplace of various molecular species. Chemical reactions occurring on the cryogenic surfaces of cosmic icy dust grains have been considered to play important roles in the formation of these species. Radical reactions are crucial because they often have low barriers and thus proceed even at low temperatures ...
openaire
Crystallization of stardust analogs under an electron flux atmosphere. [PDF]
Shohan RA +6 more
europepmc +1 more source
Shock-induced nucleation of nanophase Fe-Ni alloy and its implications for interstellar iron reservoirs. [PDF]
Velampatti Selvaraj P, Chandrasekaran V.
europepmc +1 more source
Interstellar Mapping And Acceleration Probe: The NASA IMAP Mission. [PDF]
McComas DJ +57 more
europepmc +1 more source

