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Reconstructing Fossil Sub-structures of the Galactic Disk: Clues from Abundance Patterns of Old Open Clusters and Moving Groups
G. M. De Silva, K. C. Freeman and J. Bland-Hawthorn Publications of the Astronomical Society of Australia 26(01) 11 (2009) https://doi.org/10.1071/AS08019
Fragmentation in molecular clouds and its connection to the IMF
The Density Probability Distribution in Compressible Isothermal Turbulence: Solenoidal versus Compressive Forcing
Christoph Federrath, Ralf S. Klessen and Wolfram Schmidt The Astrophysical Journal 688(2) L79 (2008) https://doi.org/10.1086/595280
The formation of the first galaxies and the transition to low-mass star formation
T. H. Greif, D. R. G. Schleicher, J. L. Johnson, et al. Proceedings of the International Astronomical Union 4(S255) 33 (2008) https://doi.org/10.1017/S1743921308024551
Gravitational fragmentation and the formation of brown dwarfs in stellar clusters
Chemically tagging the Galactic disk: abundance patterns of old open clusters
G. M. De Silva, K. C. Freeman and J. Bland-Hawthorn Proceedings of the International Astronomical Union 4(S254) 133 (2008) https://doi.org/10.1017/S1743921308027506
The First Stellar Cluster
Paul C. Clark, Simon C. O. Glover and Ralf S. Klessen The Astrophysical Journal 672(2) 757 (2008) https://doi.org/10.1086/524187
Simulating the Formation of Molecular Clouds. I. Slow Formation by Gravitational Collapse from Static Initial Conditions
Simon C. O. Glover and Mordecai‐Mark Mac Low The Astrophysical Journal Supplement Series 169(2) 239 (2007) https://doi.org/10.1086/512238
Formation of Stellar Clusters and the Importance of Thermodynamics for Fragmentation
Ralf S. Klessen, Paul C. Clark and Simon C. O. Glover Proceedings of the International Astronomical Union 3(S246) 3 (2007) https://doi.org/10.1017/S1743921308015196
On the Rapid Collapse and Evolution of Molecular Clouds
Radiation‐Hydrodynamic Simulations of Collapse and Fragmentation in Massive Protostellar Cores
Mark R. Krumholz, Richard I. Klein and Christopher F. McKee The Astrophysical Journal 656(2) 959 (2007) https://doi.org/10.1086/510664
The lower mass function of the young open cluster Blanco 1:
from 30 M$\mathsf{_{Jup}}$ to 3 M$\mathsf{_{\odot}}$
E. Moraux, J. Bouvier, J. R. Stauffer, D. Barrado y Navascués and J.-C. Cuillandre Astronomy & Astrophysics 471(2) 499 (2007) https://doi.org/10.1051/0004-6361:20066308
Simulating the Formation of Molecular Clouds. II. Rapid Formation from Turbulent Initial Conditions
Simon C. O. Glover and Mordecai‐Mark Mac Low The Astrophysical Journal 659(2) 1317 (2007) https://doi.org/10.1086/512227
The Virial Balance of Clumps and Cores in Molecular Clouds
Sami Dib, Jongsoo Kim, Enrique Vazquez‐Semadeni, Andreas Burkert and Mohsen Shadmehri The Astrophysical Journal 661(1) 262 (2007) https://doi.org/10.1086/513708
New brown dwarfs in Upper Sco using UKIDSS Galactic Cluster Survey science verification data
SPH simulations of star/planet formation triggered by cloud-cloud collisions
Spyridon Kitsionas, Anthony P. Whitworth and Ralf S. Klessen Proceedings of the International Astronomical Union 3(S249) 271 (2007) https://doi.org/10.1017/S1743921308016694
Correlations between Central Massive Objects and Their Host Galaxies: From Bulgeless Spirals to Ellipticals
Yuexing Li, Zoltan Haiman and Mordecai‐Mark Mac Low The Astrophysical Journal 663(1) 61 (2007) https://doi.org/10.1086/518398
The Mass Spectra of Cores in Turbulent Molecular Clouds and Implications for the Initial Mass Function
Javier Ballesteros‐Paredes, Adriana Gazol, Jongsoo Kim, et al. The Astrophysical Journal 637(1) 384 (2006) https://doi.org/10.1086/498228
Virginia Trimble, Markus J. Aschwanden and Carl J. Hansen Publications of the Astronomical Society of the Pacific 118(845) 947 (2006) https://doi.org/10.1086/506157
Star Formation in Isolated Disk Galaxies. II. Schmidt Laws and Efficiency of Gravitational Collapse
Yuexing Li, Mordecai‐Mark Mac Low and Ralf S. Klessen The Astrophysical Journal 639(2) 879 (2006) https://doi.org/10.1086/499350
The Jeans mass and the origin of the knee in the IMF