Results 81 to 90 of about 2,097,454 (229)
Hydrogen cyanide (HCN) molecules serve as an important tracer for the chemical evolution of elemental nitrogen in the regions of star and planet formation.
Maksim Ozhiganov +10 more
doaj +1 more source
Interstellar dust grains are enveloped by ices of frozen molecules in cold, dense regions of the interstellar medium (ISM), which are also observed in the gas phase. Whether a species is in the solid or gaseous state is governed by its binding energy (BE)
Harjasnoor Kakkar +4 more
doaj +1 more source
First detection of the pre-biotic molecule glycolonitrile (HOCH2CN) in the interstellar medium [PDF]
Shaoshan Zeng +6 more
openalex +1 more source
Interstellar ices: a possible scenario for symmetry breaking of extraterrestrial chiral organic molecules of prebiotic interest [PDF]
Louis Le Sergeant d’Hendecourt +4 more
openalex +1 more source
Excitation and emission of H, CO and HO molecules in interstellar shock waves [PDF]
D. R. Flower, G. Pineau des Forêts
openalex +1 more source
SEARCHING FOR INTERSTELLAR MOLECULE BUTATRIENYLIDENE IN REACTION C2+ C2H4 [PDF]
Shih‐Huang Lee +3 more
openalex +1 more source
Interstellar detection of the simplest aminocarbyne, H2NC: an ignored but abundant molecule [PDF]
C. Cabezas +5 more
openalex +1 more source
Diatomic molecules phosphorus monoxide (PO) and phosphorus mononitride (PN) are the main reservoirs of gas-phase phosphorus in interstellar and circumstellar environments, indicating the possibility of forming new phosphorus-bearing molecules through ...
Bifeng Zhu +8 more
doaj +1 more source
On the Origin of Infrared Bands Attributed to Tryptophan in Spitzer Observations of IC 348
Infrared emission features toward interstellar gas of the IC 348 star cluster in Perseus have been recently proposed to originate from the amino acid tryptophan.
Aditya Dhariwal +14 more
doaj +1 more source
The ALCHEMI Atlas: Principal Component Analysis Reveals Starburst Evolution in NGC 253
Molecular lines are powerful diagnostics of the physical and chemical properties of the interstellar medium (ISM). These ISM properties, which affect future star formation, are expected to differ in starburst galaxies from those of more quiescent ...
Nanase Harada +26 more
doaj +1 more source

