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HCN versus HCO+as Dense Molecular Gas Mass Tracers in Luminous Infrared Galaxies

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TURBULENCE SPECTRA FROM DOPPLER-BROADENED SPECTRAL LINES: TESTS OF THE VELOCITY CHANNEL ANALYSIS AND VELOCITY COORDINATE SPECTRUM TECHNIQUES

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THE COMPLETE SURVEY OF OUTFLOWS IN PERSEUS

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THE TEMPERATURE OF INTERSTELLAR CLOUDS FROM TURBULENT HEATING

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Formation of complex chemical species in astrochemistry (a review)

V. I. Shematovich
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TEMPORAL SMEARING OF TRANSIENT RADIO SOURCES BY THE INTERGALACTIC MEDIUM

Jean-Pierre Macquart and Jun Yi Koay
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Intermittency of interstellar turbulence: parsec-scale coherent structure of intense, velocity shear

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Models of turbulent dissipation regions in the diffuse interstellar medium

B. Godard, E. Falgarone and G. Pineau des Forêts
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VELOCITY FIELD OF COMPRESSIBLE MAGNETOHYDRODYNAMIC TURBULENCE: WAVELET DECOMPOSITION AND MODE SCALINGS

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Studying Turbulence Using Doppler‐broadened Lines: Velocity Coordinate Spectrum

A. Lazarian and D. Pogosyan
The Astrophysical Journal 652 (2) 1348 (2006)
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Rotational excitation of simple polar molecules by H2and electrons in diffuse clouds

H. S. Liszt
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Dissipative structures of diffuse molecular gas

P. Hily-Blant, E. Falgarone and J. Pety
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Imaging galactic diffuse gas: bright, turbulent CO surrounding the line of sight to NRAO150

J. Pety, R. Lucas and H. S. Liszt
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ANISOTROPY LENGTHENS THE DECAY TIME OF TURBULENCE IN MOLECULAR CLOUDS

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Radiative Transfer in Molecular Clouds

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Low sulfur depletion in the Horsehead PDR

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Properties and Selected Implications of Magnetic Turbulence for Interstellar Medium, Local Bubble and Solar Wind

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From the Outer Heliosphere to the Local Bubble

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A HIGH-RESOLUTION ISOTOPIC STUDY OF THE ROTATIONAL SPECTRUM OF c -C 3 H 2

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The Role of Neutral Hydrogen in Setting the Abundances of Molecular Species in the Milky Way’s Diffuse Interstellar Medium. II. Comparison between Observations and Theoretical Models

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The Role of Neutral Hydrogen in Setting the Abundances of Molecular Species in the Milky Way’s Diffuse Interstellar Medium. I. Observational Constraints from ALMA and NOEMA

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