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20072025
most citedThe Star Formation Rate of Turbulent Magnetized Clouds: Comparing Theory, Simulations, and Observations

779 citations · 13.3k across the 229 of their papers we have counts for

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Showing 2021Show all

23 papers · 1 filter

astro-ph.GA2021★ 18 cited

Non-ideal MHD simulations of subcritical prestellar cores with non-equilibrium chemistry

Aris Tritsis, Christoph Federrath, Karen Willacy +1

Non-ideal magnetohydrodynamic (MHD) effects are thought to be gravity's closest ally in overcoming the support of magnetic fields and in forming stars. Here, we modify the publicly…

astro-ph.GA2021★ 19 cited

A new method for measuring the 3D turbulent velocity dispersion of molecular clouds

Madeleine Stewart, Christoph Federrath

The structure and star formation activity of a molecular cloud are fundamentally linked to its internal turbulence. However, accurately measuring the turbulent velocity dispersion…

astro-ph.GA2021★ 47 cited

Impact of relativistic jets on the star formation rate: a turbulence-regulated framework

Ankush Mandal, Dipanjan Mukherjee, Christoph Federrath +4

We apply a turbulence-regulated model of star formation to calculate the star formation rate (SFR) of dense star-forming clouds in simulations of jet-ISM interactions. The method i…

astro-ph.GA2021★ 24 cited

First extragalactic measurement of the turbulence driving parameter: ALMA observations of the star-forming region N159E in the Large Magellanic Cloud

Piyush Sharda, Shyam H. Menon, Christoph Federrath +13

Studying the driving modes of turbulence is important for characterizing the impact of turbulence in various astrophysical environments. The driving mode of turbulence is parameter…

astro-ph.GA2021★ 3 cited

Quantifying stochasticity-driven uncertainties in H II region metallicities

Raghav Arora, Mark R. Krumholz, Christoph Federrath

With the advent of Integral Field Units (IFUs), surveys can now measure metallicities across the discs of nearby galaxies at scales pc. At such small scales, many o…

astro-ph.GA2021★ 26 cited

The Effects of Magnetic Fields and Outflow Feedback on the Shape and Evolution of the Density PDF in Turbulent Star-Forming Clouds

Sabrina M. Appel, Blakesley Burkhart, Vadim A. Semenov +2

Using a suite of 3D hydrodynamical simulations of star-forming molecular clouds, we investigate how the density probability distribution function (PDF) changes when including gravi…