Spiral magneto-electron waves in the interstellar gas dynamics
We discuss possible observational consequences resulting from the propagation of transverse magneto-electron waves in the interstellar medium. We briefly describe the magnetohydrodynamics model for the cyclotron waves with the emphasis on their analogy ...
양종만
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Rotational Characterization of Four-Ring Polycyclic Aromatic Hydrocarbons: Toward the Detection of Fluoranthene and Cyanofluoranthene in Space. [PDF]
Villar-Castro D +10 more
europepmc +1 more source
Grain alignment in dense interstellar environments: spectropolarimetry of the 4.67-μm CO-ice feature in the field star Elias 16 (Taurus dark cloud) [PDF]
J. H. Hough +4 more
openalex +1 more source
Erratum: Molecular Hydrogen in Interstellar Dark Clouds
Mark Allen, G. Wilse Robinson
openaire +1 more source
Cryogenic Bottom-up Formation of the Benzene Cation from Acetylene in Helium Nanodroplets. [PDF]
Foitzik F +5 more
europepmc +1 more source
Interstellar dust in the rho OPH dark cloud.
L. Carrasco, S. E. Strom, K. M. Strom
openaire +1 more source
Laboratory Investigation of Simultaneous Ultraviolet Photoprocessing and Temperature-Programmed Desorption of Interstellar Ice Analogs. [PDF]
Sarver CC, Walker CE, Widicus Weaver SL.
europepmc +1 more source
Thermal Synthesis of Carbamic Acid and Its Dimer in Interstellar Ices: A Reservoir of Interstellar Amino Acids. [PDF]
Marks JH +6 more
europepmc +1 more source
Coupling laboratory FTIR data with PROCODA kinetic modeling for the radiolysis of frozen formic acid using swift ions. [PDF]
Moraes L, Fargnoli CM, Pilling S.
europepmc +1 more source
On the constant surface density in dark matter galaxies and interstellar molecular clouds
9 pages, 2 figuresCumulative observational evidence confirm that the surface density of dark matter (DM) halos mu_{0 D} = r_0 rho_0, (r_0 and rho_0 are the halo core radius and central density, respectively), is nearly constant and independent of galaxy ...
de Vega, H. J., Sanchez, N. G.
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