activity
20052023
most citedThe CO-to-H2 Conversion Factor and Dust-to-Gas Ratio on Kiloparsec Scales in Nearby Galaxies

601 citations · 3.6k across the 47 of their papers we have counts for

collaborators

47 papers

astro-ph.GA2023

A reproduction of the Milky Way's Faraday rotation measure map in galaxy simulations from global to local scales

Stefan Reissl, Ralf S. Klessen, Eric W. Pellegrini +6

Magnetic fields are of critical importance for our understanding of the origin and long-term evolution of the Milky Way. This is due to their decisive role in the dynamical evoluti…

astro-ph.IM2022★ 3 cited

Validating the Local Volume Mapper acquisition and guiding hardware

Maximilian Häberle, Thomas M. Herbst, Peter Bizenberger +13

The Local Volume Mapper (LVM) project is one of three surveys that form the Sloan Digital Sky Survey V. It will map the interstellar gas emission in a large fraction of the souther…

astro-ph.GA2022★ 1 cited

30 Doradus, the double stellar birth scenario by -body \& \textsc{warpfield} clouds

R. Domínguez, Eric W. Pellegrini, Ralf S. Klessen +1

We study the evolution of embedded star clusters as possible progenitors to reproduce 30 Doradus, specifically the compact star cluster known as R136 and its surrounding stellar fa…

astro-ph.GA2022★ 17 cited

Emission-line diagnostics of HII regions using conditional Invertible Neural Networks

Da Eun Kang, Eric W. Pellegrini, Lynton Ardizzone +4

Young massive stars play an important role in the evolution of the interstellar medium (ISM) and the self-regulation of star formation in giant molecular clouds (GMCs) by injecting…

astro-ph.GA2021★ 5 cited

Limits to Ionization-Parameter Mapping as a Diagnostic of HII Region Optical Depth

Amit N. Sawant, Eric W. Pellegrini, M. S. Oey +2

We employ ionization-parameter mapping (IPM) to infer the optical depth of HII regions in the northern half of M33. We construct [OIII]/[OII] and [OIII]/[SII]$…

astro-ph.GA2020★ 16 cited

Less than the sum of its parts: the dust-corrected H luminosity of star-forming galaxies explored at different spatial resolutions with MaNGA and MUSE

N. Vale Asari, V. Wild, A. L. de Amorim +10

The H and H emission line luminosities measured in a single integrated spectrum are affected in non-trivial ways by point-to-point variations in dust attenuation in a galaxy.…