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Cited article:
Yueh-Ning Lee, Patrick Hennebelle
A&A, 611 (2018) A89
Published online: 2018-04-04
This article has been cited by the following article(s):
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Effects of the environment and feedback physics on the initial mass function of stars in the STARFORGE simulations
Dávid Guszejnov, Michael Y Grudić, Stella S R Offner, Claude-André Faucher-Giguère, Philip F Hopkins and Anna L Rosen
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What Is the Role of Stellar Radiative Feedback in Setting the Stellar Mass Spectrum?
Patrick Hennebelle, Benoît Commerçon, Yueh-Ning Lee and Gilles Chabrier
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The Astrophysical Journal 883 (2) 140 (2019)
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Density profile evolution during prestellar core collapse: collapse starts at the large scale
Gilberto C Gómez, Enrique Vázquez-Semadeni and Aina Palau
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Numerical Methods for Simulating Star Formation
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Star cluster formation in clouds with externally driven turbulence
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Cloud Properties and Correlations with Star Formation in Self-consistent Simulations of the Multiphase ISM
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Astronomy & Astrophysics 622 A125 (2019)
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A dual power-law distribution for the stellar initial mass function
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Core and stellar mass functions in massive collapsing filaments
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Detection and characterisation of 54 massive companions with the SOPHIE spectrograph
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Influence of protostellar jets and HII regions on the formation and evolution of stellar clusters
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From Diffuse Gas to Dense Molecular Cloud Cores
Javier Ballesteros-Paredes, Philippe André, Patrick Hennebelle, Ralf S. Klessen, J. M. Diederik Kruijssen, Mélanie Chevance, Fumitaka Nakamura, Angela Adamo and Enrique Vázquez-Semadeni
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Can magnetized turbulence set the mass scale of stars?
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Strong dependence of the physical properties of cores on spatial resolution in observations and simulations
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