activity
20092026
most citedHow Universal is the SFR - H2 Relation?

69 citations · 142 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2026

GLOW II: A Census of Oxygen in Low-Mass Galaxies

Kristen B. W. McQuinn, O. Grace Telford, Andrey V. Kravtsov +12

Oxygen is forged by stars and redistributed through galaxies by feedback-driven outflows, leaving a record of star formation and the baryon cycle imprinted on its present-day abund…

astro-ph.IM2025

Picture an Astronomer: Best Practices for Retaining Talent in Astrophysics

Ava Polzin, Katherine E. Whitaker, C. Megan Urry +85

Women are consistently underrepresented in astrophysics yet are simultaneously subject to disproportionate attrition at every career stage. This disparity between demonstrated effi…

astro-ph.GA2025★ 1 cited

What Sets the Metallicity of Ultra-Faint Dwarfs?

Vance Wheeler, Andrey Kravtsov, Anirudh Chiti +2

We use intergalactic medium (IGM) metallicity distributions from several state-of-the-art cosmological simulations of Milky Way analogs and a semi-analytic model of ultra-faint dwa…

astro-ph.GA2024★ 8 cited

On the universality of star formation efficiency in galaxies

Ava Polzin, Andrey V. Kravtsov, Vadim A. Semenov +1

We analyze high-resolution hydrodynamics simulations of an isolated disk dwarf galaxy with an explicit model for unresolved turbulence and turbulence-based star formation prescript…

astro-ph.GA2023★ 7 cited

Modeling molecular hydrogen in low metallicity galaxies

Ava Polzin, Andrey V. Kravtsov, Vadim A. Semenov +1

We use a suite of hydrodynamics simulations of the interstellar medium (ISM) within a galactic disk, which include radiative transfer, a non-equilibrium model of molecular hydrogen…

astro-ph.CO2010★ 69 cited

How Universal is the SFR - H2 Relation?

R. Feldmann, N. Y. Gnedin, A. V. Kravtsov

It is a well established empirical fact that the surface density of the star formation rate, Sigma_SFR, strongly correlates with the surface density of molecular hydrogen, Sigma_H2…