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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 2022Show all

22 papers · 1 filter

astro-ph.SR2022

Hyperion: The origin of the stars A far-UV space telescope for high-resolution spectroscopy over wide fields

Erika Hamden, David Schiminovich, Shouleh Nikzad +30

We present Hyperion, a mission concept recently proposed to the December 2021 NASA Medium Explorer announcement of opportunity. Hyperion explores the formation and destruction of m…

astro-ph.GA2022

Can pre-supernova winds from massive stars enrich the interstellar medium with nitrogen at high redshift?

Arpita Roy, Mark R. Krumholz, Michael A. Dopita +3

Understanding the nucleosynthetic origin of nitrogen and the evolution of the N/O ratio in the interstellar medium is crucial for a comprehensive picture of galaxy chemical evoluti…

astro-ph.HE2022★ 5 cited

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

Matt A. Roth, Mark R. Krumholz, Roland M. Crocker +1

The total luminosity and spectral shape of the non-thermal emission produced by cosmic rays depends on their interstellar environment, a dependence that gives rise to correlations…

astro-ph.GA2022★ 13 cited

The impact of carbon and oxygen abundances on the metal-poor initial mass function

Piyush Sharda, Anish M. Amarsi, Kathryn Grasha +5

Star formation models predict that the metal-poor initial mass function (IMF) can be substantially different from that observed in the metal-rich Milky Way. This changeover occurs…

astro-ph.GA2022★ 20 cited

The cosmic ray ionisation and -ray budgets of star-forming galaxies

Mark R. Krumholz, Roland M. Crocker, Stella S. R. Offner

Cosmic rays in star-forming galaxies are a dominant source of both diffuse -ray emission and ionisation in gas too deeply shielded for photons to penetrate. Though the cosmic ra…

astro-ph.GA2022★ 51 cited

Outflows Driven by Direct and Reprocessed Radiation Pressure in Massive Star Clusters

Shyam H. Menon, Christoph Federrath, Mark R. Krumholz

We use three-dimensional radiation hydrodynamic (RHD) simulations to study the formation of massive star clusters under the combined effects of direct ultraviolet (UV) and dust-rep…