Results 91 to 100 of about 1,388 (238)
Formation of Methanol via Fischer‐Tropsch Catalysis by Cosmic Iron Sulphide
Periodic quantum mechanical simulations evidence the potentiality to synthesise methanol through a Fischer‐Tropsch mechanism in different astrophysical environments facilitated by the catalytic properties of cosmic FeS grains, which are enhanced by the presence of naturally‐occurring point surface defects.
Berta Martinez‐Bachs +3 more
wiley +1 more source
Thermal and maser molecular emission in infrared dark clouds [PDF]
Доклад посвящен наблюдательным проявлениям процесса звездообразования в плотных темных облаках в межзвездной среде Галактики. Приведены примеры таких проявлений, дан краткий обзор характеристик молекулярных облаков.
Шахворостова, Н. Н. +1 more
core +1 more source
Rotational excitation of methanol by helium at interstellar temperatures [PDF]
Calculations have been performed to obtain accurate cross-sections and thermally averaged rate coefficients for the rotational excitation of methanol by helium, using the Coupled States quantum-mechanical approach. Transitions within the ground and first
Pottage, James
core
The Magnetic Field in Quiescent Star-forming Filament G16.96+0.27
We present 850 μ m thermal dust polarization observations with a resolution of 14.″4 (∼0.13 pc) toward an infrared dark cloud G16.96+0.27 using James Clerk Maxwell Telescope/POL-2.
Qi-Lao Gu +22 more
doaj +1 more source
The collective origin of spiral structures in disk galaxies
After almost fifty years the origin of spiral arms in disk galaxies remains one of the major unsolved problems in astrophysics. Recent attempts have indicated that substructures in the dark matter halos of galaxies could induce spiral patterns in disks ...
Hernquist L. +2 more
doaj +1 more source
A comprehensive 3D model of the central 300 pc of the Milky Way, the Central Molecular Zone (CMZ) is of fundamental importance in understanding energy cycles in galactic nuclei, since the 3D structure influences the location and intensity of star ...
Dani Lipman +17 more
doaj +1 more source
Grain growth, optical polarisation, and extinction in interstellar clouds
Increases in the wavelength of maximum polarization and the ratio of total to selective extinction are generally assumed to be the result of grain growth in interstellar clouds.
Jones, A. P.
core
Methanol as a diagnostic tool of interstellar clouds
Context.Fundamental properties of interstellar clouds must be known to investigate the initial conditions of star formation within them and the interaction of newly formed stars with their environment.
S. Leurini +3 more
core +1 more source
In recent years, a significant number of oxygen-bearing complex organic molecules (COMs) have been detected in the gas phase of cold dark clouds such as TMC-1.
Yang Lu +4 more
doaj +1 more source
Supersonic waves of magnetization in dark interstellar molecular clouds
We suggest that supersonic linewidths inferred from recent measurements of magnetic fields toward the core position in dark interstellar molecular clouds may be due to transverse waves of magnetization propagating in a poorly ionized, magnetically ...
양종만
core

