activity
20022026
most citedGas Stripping in Simulated Galaxies with a Multiphase ISM

246 citations · 3.5k across the 80 of their papers we have counts for

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Showing astro-ph.COShow all

7 papers · 1 filter

astro-ph.CO2024

The Effects of AGN Feedback on the Lyman- Forest Flux Power Spectrum

Megan Taylor Tillman, Blakesley Burkhart, Stephanie Tonnesen +2

We study the effects of AGN feedback on the Lyman- forest 1D flux power spectrum (P1D). Using the Simba cosmological-hydrodynamic simulations, we examine the impact that adding…

astro-ph.CO2022★ 43 cited

Cosmology with one galaxy?

Francisco Villaescusa-Navarro, Jupiter Ding, Shy Genel +10

Galaxies can be characterized by many internal properties such as stellar mass, gas metallicity, and star-formation rate. We quantify the amount of cosmological and astrophysical i…

astro-ph.CO2017★ 16 cited

Probing the Dependence of the Intergalactic Medium on Large Scale Environment Using the Low Redshift Lyman Alpha Forest

Stephanie Tonnesen, Britton D. Smith, Juna Kollmeier +1

We examine the statistics of the low-redshift Ly-alpha forest in an adaptive mesh refinement hydrodynamic cosmological simulation of sufficient volume to include distinct large-sca…

astro-ph.CO2012★ 132 cited

Star Formation in Ram Pressure Stripped Tails

Stephanie Tonnesen, Greg L. Bryan

We investigate the impact of star formation and feedback on ram pressure stripping using high-resolution adaptive mesh simulations, building on a previous series of papers that sys…

astro-ph.CO2011★ 40 cited

Effects on Galaxy Evolution: Pair Interactions versus Environment

Stephanie Tonnesen, Renyue Cen

In a hierarchical universe, mergers may be an important mechanism not only in increasing the mass of galaxies but also in driving the color and morphological evolution of galaxies.…

astro-ph.CO2011★ 46 cited

How To Light It Up: Simulating Ram-Pressure Stripped X-ray Bright Tails

Stephanie Tonnesen, Greg L. Bryan, Rena Chen

Some tails of ram-pressure stripped galaxies are detected in HI, some in Halpha, and some in X-ray (but never all three so far). We use numerical simulations to probe the condition…