Molecular Clouds: Internal Properties, Turbulence, Star Formation and Feedback
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- Type
- article
- Published
- 2012-08-01
- Cited by
- 10
- References
- 88
- Access
- Open access
- OpenAlex
- https://openalex.org/W2166672701
- Semantic Scholar
- https://api.semanticscholar.org/CorpusID:119253736
Keywords
Star formation, Molecular cloud, Physics, Astrophysics, Stars
References
- Protostars and Planets VI
- Physics of the Interstellar and Intergalactic Medium
- The initial conditions of stellar protocluster formation - I. A catalogue of Spitzer dark clouds
- The Genesis of Super Star Clusters as Self-Gravitating HII Regions
- High CO depletion in southern infrared dark clouds
- Molecular cloud evolution – IV. Magnetic fields, ambipolar diffusion and the star formation efficiency
- STELLAR FEEDBACK IN MOLECULAR CLOUDS AND ITS INFLUENCE ON THE MASS FUNCTION OF YOUNG STAR CLUSTERS
- STAR FORMATION IN DISK GALAXIES. I. FORMATION AND EVOLUTION OF GIANT MOLECULAR CLOUDS VIA GRAVITATIONAL INSTABILITY AND CLOUD COLLISIONS
- THE GLOBAL EVOLUTION OF GIANT MOLECULAR CLOUDS. II. THE ROLE OF ACCRETION
- Models of Massive Molecular Clouds
- Super Star Cluster Velocity Dispersions and Virial Masses in the M82 Nuclear Starburst
- MAPPING LARGE-SCALE CO DEPLETION IN A FILAMENTARY INFRARED DARK CLOUD
- A Preliminary Study of the Orion Nebula Cluster Structure and Dynamics
- The Elongations and Supersonic Motions of Molecular Clouds
- Slow Star Formation in Dense Gas: Evidence and Implications
- THE “NESSIE” NEBULA: CLUSTER FORMATION IN A FILAMENTARY INFRARED DARK CLOUD
- C-12/C-13 isotope ratio across the Galaxy from observations of C-13/O-18 in molecular clouds
- Fragmentation and mass segregation in the massive dense cores of Cygnus X
- DETAILED NUMERICAL SIMULATIONS ON THE FORMATION OF PILLARS AROUND H ii REGIONS
- Dense Gas and Star Formation: Characteristics of Cloud Cores Associated with Water Masers
Cited by
- Kinematics and physical properties of a highly filamentary Infrared Dark Cloud
- Dense cloud cores revealed by CO in the low metallicity dwarf galaxy WLM
- THE GALACTIC CENSUS OF HIGH- AND MEDIUM-MASS PROTOSTARS. II. LUMINOSITIES AND EVOLUTIONARY STATES OF A COMPLETE SAMPLE OF DENSE GAS CLUMPS
- KILOPARSEC-SCALE SIMULATIONS OF STAR FORMATION IN DISK GALAXIES. I. THE UNMAGNETIZED AND ZERO-FEEDBACK LIMIT
- From Interstellar Clouds to Stars
- Formation and Evolution of Magnetised and Turbulent Molecular Clouds : Varying Initial Conditions and the Role of Stellar Feedback
- Investigation into triggered star formation by radiative driven implosion
- Dynamical cooling of galactic discs by molecular cloud collisions - origin of giant clumps in gas-rich galaxy discs
- Th Dynamics of Star Cluster Formation
- The Raw Material of Cluster Formation: Observational Constraints
- The Galactic Census of High- and Medium-mass Protostars. II. Luminosities and Evolutionary States of a Complete Sample of Dense Gas Clumps
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