Mark Krumholz

Professor

Australian National University

Australia

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About

Professor Mark Krumholz is a faculty member at the Australian National University in Australia. His research primarily focuses on the dynamics of galaxies, stellar actions, and the chemical evolution of the universe, as evidenced by his recent articles on orbit reconstruction, gas-phase metallicities, and the dynamics of molecular clouds. He is also involved in exploring the roles of pressure in galactic structures and the distribution of metals across galaxies.

Articles (20)

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2025

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2023

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2023

Collaborators (15)

Jan Forbrich

University of Hertfordshire

UNITED KINGDOM

Mark Krumholz

Research Interests

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About

Articles (20)

Exploring the chemical content of Galaxies using the SAMI Zoom Survey: a data release of 92 spatially resolved H ii regions in nearby galaxies

Element Nucleosynthetic Origins from Abundance Spatial Distributions beyond the Milky Way

Fundamental limits to orbit reconstruction due to non-conservation of stellar actions in a Milky Way-like simulation

Optimal strategies for measuring gas-phase metallicities in intermediate-redshift non-AGN and AGN-host galaxies using future instrumentation

Differential virial analysis: a new technique to determine the dynamical state of molecular clouds

Wind of change: Faraday rotation in a simulated Large Magellanic Cloud

Understanding the mechanisms behind the distribution of galactic metals

The Role of Pressure in the Structure and Stability of GMCs in the Andromeda Galaxy

QUOKKA-based understanding of outflows (QED) – III. Outflow loading and phase structure as a function of galactic environment

quokka-based understanding of outflows (QED) – II. X-ray metallicity gradients as a signature of galactic wind metal loading

Correction to ‘The impact of carbon and oxygen abundances on the metal-poor initial mass function'

Gas Accretion Can Drive Turbulence in Galaxies

Correction to: Cosmic Ray Interstellar Propagation Tool using Itô Calculus (criptic): Software for simultaneous calculation of cosmic ray transport and observational signatures

Constraining the LyC escape fraction from LEGUS star clusters with SIGNALS H ii region observations: a pilot study of NGC 628

Direct observations of the atomic-molecular phase transition in the Milky Way’s nuclear wind

Spatially resolved dust properties and quasar-galaxy decomposition of a hyper-luminous infrared galaxy at z = 4.4

congruents (COsmic ray, Neutrino, Gamma-ray, and Radio Non-Thermal Spectra) – I. A predictive model for galactic non-thermal emission

Outflows driven by direct and reprocessed radiation pressure in massive star clusters

The global structure of magnetic fields and gas in simulated Milky Way-analogue galaxies

The sub-critical illusion: synthetic Zeeman effect observations from galactic zoom-in simulations

Collaborators (15)

Jan Forbrich

Andrew Battisti

Emily Wisnioski

Takafumi Tsukui

D Yong

Thomas Nordlander

Roland Crocker

Greg Bryan

Lucia Armillotta

Christoph Federrath

Sarah Sweet

Angel Lopez-Sanchez

Matt L Sampson

Anish Mayur Amarsi

Anna Faye McLeod

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