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19982026
most citedA General Theory of Turbulence-Regulated Star Formation, From Spirals to ULIRGs

1.1k citations · 24.6k across the 330 of their papers we have counts for

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Showing 2013Show all

17 papers · 1 filter

astro-ph.GA2013★ 72 cited

Formation of Molecular Clouds and Global Conditions for Star Formation

Clare L. Dobbs, Mark R. Krumholz, Javier Ballesteros-Paredes +6

Giant molecular clouds (GMCs) are the primary reservoirs of cold, star-forming molecular gas in the Milky Way and similar galaxies, and thus any understanding of star formation mus…

astro-ph.CO2013★ 100 cited

On the origin of the fundamental metallicity relation and the scatter in galaxy scaling relations

John C. Forbes, Mark R. Krumholz, Andreas Burkert +1

We present a simple toy model to understand what sets the scatter in star formation and metallicity of galaxies at fixed mass. The scatter ultimately arises from the intrinsic scat…

astro-ph.CO2013★ 165 cited

The Star Formation Law in Molecule-Poor Galaxies

Mark R. Krumholz

In this paper, I investigate the processes that regulate the rate of star formation in regions of galaxies where the neutral interstellar medium is predominantly composed of non-st…

astro-ph.SR2013★ 160 cited

The Role of Stellar Feedback in the Dynamics of HII Regions

Laura A. Lopez, Mark R. Krumholz, Alberto D. Bolatto +3

Stellar feedback is often cited as the biggest uncertainty in galaxy formation models today. This uncertainty stems from a dearth of observational constraints as well as the great…

astro-ph.GA2013★ 282 cited

The AGORA High-Resolution Galaxy Simulations Comparison Project

Ji-hoon Kim, Tom Abel, Oscar Agertz +43

We introduce the AGORA project, a comprehensive numerical study of well-resolved galaxies within the LCDM cosmology. Cosmological hydrodynamic simulations with force resolutions of…

astro-ph.CO2013★ 145 cited

Balance among gravitational instability, star formation, and accretion determines the structure and evolution of disk galaxies

John C. Forbes, Mark R. Krumholz, Andreas Burkert +1

Over the past 10 Gyr, star-forming galaxies have changed dramatically, from clumpy and gas rich, to rather quiescent stellar-dominated disks with specific star formation rates lowe…