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Nature|September 2, 2014
Early turbulent mixing as the origin of chemical homogeneity in open star clustersYi Feng, Mark R KrumholzNature|February 29, 2008
A minimum column density of 1 g cm(-2) for massive star formationMark R Krumholz, Christopher F McKeeMonthly Notices of the Royal Astronomical Society|October 7, 2022
Environmental variation of the low-mass IMFTabassum S Tanvir, Mark R Krumholz, Christoph FederrathMonthly Notices of the Royal Astronomical Society|August 15, 2020
Distribution and kinematics of 26Al in the Galactic discYusuke Fujimoto, Mark R Krumholz, Shu-Ichiro InutsukaMonthly Notices of the Royal Astronomical Society|January 22, 2019
slug IV: a novel forward-modelling method to derive the demographics of star clustersMark R Krumholz, Angela Adamo, Michele Fumagalli, et al.Monthly Notices of the Royal Astronomical Society|May 23, 2024
An asymptotically correct implicit-explicit time integration scheme for finite volume radiation-hydrodynamicsChong-Chong He, Benjamin D Wibking, Mark R KrumholzMonthly Notices of the Royal Astronomical Society|April 8, 2020
The life cycle of the Central Molecular Zone - II. Distribution of atomic and molecular gas tracersLucia Armillotta, Mark R Krumholz, Enrico M Di TeodoroNature|November 18, 2005
The formation of stars by gravitational collapse rather than competitive accretionMark R Krumholz, Christopher F McKee, Richard I KleinMonthly Notices of the Royal Astronomical Society|February 27, 2023
The cosmic ray ionization and γ-ray budgets of star-forming galaxiesMark R Krumholz, Roland M Crocker, Stella S R OffnerNature|September 16, 2021
The diffuse γ-ray background is dominated by star-forming galaxiesMatt A Roth, Mark R Krumholz, Roland M Crocker, et al.Pageof 2