149 citations · 592 across the 11 of their papers we have counts for
11 papers
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…
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…
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.…
WARPFIELD-EMP: The Self-Consistent Prediction of Emission Lines from Evolving HII Regions in Dense Molecular Clouds
Eric W. Pellegrini, Daniel Rahner, Stefan Reissl +4
We present the {\sc warpfield} emission predictor, {\sc warpfield-emp}, which couples the 1D stellar feedback code {\sc warpfield} with the {\sc cloudy} \hii region/PDR code and th…
SIGNALS: I. Survey Description
L. Rousseau-Nepton, R. P. Martin, C. Robert +60
SIGNALS, the Star formation, Ionized Gas, and Nebular Abundances Legacy Survey, is a large observing program designed to investigate massive star formation and HII regions in a sam…
WARPFIELD Population Synthesis: The physics of (extra-)Galactic star formation and feedback driven cloud structure and emission from sub-to-kpc scales
E. W. Pellegrini, S. Reissl, D. Rahner +5
We present a novel method to model galactic scale star formation and the resulting emission from star clusters and the multi-phase interstellar medium. We combine global parameters…