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Reaction Mechanisms to Enhance Chemical Complexity in Cold, Dark Interstellar Clouds
2023The cold, dark, interstellar cloud TMC-1 is home to more than 148 known molecules, and possibly many more. To understand the formation and destruction of these molecules, we present detailed theoretical work combined with a vast chemical kinetic model, Nautilus.
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On the constant surface density in dark matter galaxies and interstellar molecular clouds
2009Cumulative 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 luminosity for a high number of galactic systems (spirals, dwarf irregular and spheroidals, elliptics).
de Vega, H. J., Sanchez, N. G.
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ORTHO-H2 AND THE AGE OF INTERSTELLAR DARK CLOUDS
Astrophysical Journal Letters, 2011Laurent Pagani, Evelyne Roueff
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Cold Dark Clouds: The Initial Conditions for Star Formation
Annual Review of Astronomy and Astrophysics, 2007Mario Tafalla, Edwin Bergin
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Local interstellar medium kinematics towards the Southern Coalsack and Chamaeleon-Musca dark clouds
Monthly Notices of the Royal Astronomical Society, 2004Gabriel A. P. Franco
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Radio observations of interstellar CN toward diffuse clouds, dark clouds, and circumstellar clouds.
Astrophysical Journal, 1978G R Knapp
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