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Relative Velocities between 13CO Structures within 12CO Molecular Clouds
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Gravity versus Magnetic Fields in Forming Molecular Clouds
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Statistical properties and correlation length in star-forming molecular clouds
TIMES. I. A Systematic Observation in Multiple Molecular Lines toward the Orion A and Ophiuchus Clouds
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Testing the turbulent origin of the stellar initial mass function
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Diagnosing Turbulence in the Neutral and Molecular Interstellar Medium of Galaxies
Neal J. Evans II, Mark Heyer, Marc-Antoine Miville-Deschênes, Quang Nguyen-Luong and Manuel Merello The Astrophysical Journal 920(2) 126 (2021) https://doi.org/10.3847/1538-4357/ac1425
The Cloud Factory II: gravoturbulent kinematics of resolved molecular clouds in a galactic potential
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CO Outflow Candidates toward the W3/4/5 Complex. II. Feedback from Candidate Outflows
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∗
H. Übler, R. Genzel, E. Wisnioski, N. M. Förster Schreiber, T. T. Shimizu, S. H. Price, L. J. Tacconi, S. Belli, D. J. Wilman, M. Fossati, J. T. Mendel, R. L. Davies, A. Beifiori, R. Bender, G. B. Brammer, A. Burkert, J. Chan, R. I. Davies, M. Fabricius, A. Galametz, R. Herrera-Camus, P. Lang, D. Lutz, I. G. Momcheva, T. Naab, et al. The Astrophysical Journal 880(1) 48 (2019) https://doi.org/10.3847/1538-4357/ab27cc
Effects of infall and outflow on massive star-forming regions
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The CARMA–NRO Orion Survey: Statistical Signatures of Feedback in the Orion A Molecular Cloud
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How do velocity structure functions trace gas dynamics in simulated molecular clouds?
Global hierarchical collapse in molecular clouds. Towards a comprehensive scenario
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Molecular Gas toward the Gemini OB1 Molecular Cloud Complex. II. CO Outflow Candidates with Possible WISE Associations
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ALMA Observations of a Quiescent Molecular Cloud in the Large Magellanic Cloud
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Diversity of dwarf galaxy IR-submm emission patterns: CLUES from hydrodynamical simulations
Isabel M. E. Santos-Santos, Rosa Domínguez-Tenreiro, Gian Luigi Granato, Chris B. Brook and Aura Obreja Astronomy & Astrophysics 603 A4 (2017) https://doi.org/10.1051/0004-6361/201629426
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Fast Molecular Cloud Destruction Requires Fast Cloud Formation
Probes of turbulent driving mechanisms in molecular clouds from fluctuations in synchrotron intensity
C. A. Herron, C. Federrath, B. M. Gaensler, et al. Monthly Notices of the Royal Astronomical Society 466(2) 2272 (2017) https://doi.org/10.1093/mnras/stw3319
On the effective turbulence driving mode of molecular clouds formed in disc galaxies
Keitaro Jin, Diane M. Salim, Christoph Federrath, et al. Monthly Notices of the Royal Astronomical Society 469(1) 383 (2017) https://doi.org/10.1093/mnras/stx737
Cloud-scale ISM Structure and Star Formation in M51
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Magnetohydrodynamical simulation of the formation of clumps and filaments in quiescent diffuse medium by thermal instability
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On the universality of interstellar filaments: theory meets simulations and observations
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The role of turbulence, magnetic fields and feedback for star formation
GRAVITATIONAL CONTRACTION VERSUS SUPERNOVA DRIVING AND THE ORIGIN OF THE VELOCITY DISPERSION–SIZE RELATION IN MOLECULAR CLOUDS
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PRINCIPAL COMPONENT ANALYSIS STUDIES OF TURBULENCE IN OPTICALLY THICK GAS
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AN EVOLUTIONARY MODEL FOR COLLAPSING MOLECULAR CLOUDS AND THEIR STAR FORMATION ACTIVITY. II. MASS DEPENDENCE OF THE STAR FORMATION RATE
Testing assumptions and predictions of star formation theories
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Prospects of turbulence studies in high-energy density laser-generated plasma: Numerical investigations in two dimensions