31 citations · 141 across the 11 of their papers we have counts for
11 papers
The Star Formation Factory revisited I. The impact of metallicity on collapsing star-forming clouds
S. Jiménez, D. Kománek, R. Wünsch +4
Context. Stellar feedback regulates star formation and shapes the interstellar medium, yet its role during the collapse of molecular clouds remains uncertain over a wide range of i…
Molecular gas properties in young stellar clusters with a suppressed star cluster wind
Sergiy Silich, Jean Turner, Jonathan Mackey +1
In compact and dense star-forming clouds a global star cluster wind could be suppressed. In this case the stellar feedback is unable to expel the leftover gas from the cluster. You…
Dust Grain Growth & Dusty Supernovae in Low-Metallicity Molecular Clouds
Sergio Martínez-González, Richard Wünsch, Guillermo Tenorio-Tagle +3
We present 3-D hydrodynamical models of the evolution of superbubbles powered by stellar winds and supernovae from young coeval massive star clusters within low metallicity ($Z = 0…
X-ray emission from star cluster winds in starburst galaxies
Annika Franeck, Richard Wünsch, Sergio Martínez-González +5
Inspired by the excess soft X-ray emission recently detected in Green Pea galaxies, we model the soft X-ray emission (0.5 - 2.0 keV) of hot gas from star cluster winds. By combinin…
On the early evolution of massive star clusters: the case of cloud D1 and its embedded cluster in NGC 5253
Sergiy Silich, Guillermo Tenorio-Tagle, Sergio Martinez-Gonzalez +1
We discuss a theoretical model for the early evolution of massive star clusters and confront it with the ALMA, radio and infrared observations of the young stellar cluster highly o…
Can Dust Injected by SNe Explain the NIR-MIR Excess in Young Massive Stellar Clusters?
Sergio Martinez-Gonzalez, Richard Wünsch, Jan Palouš
We present a physically-motivated model involving the different processes affecting supernova dust grains as they are incorporated into the thermalized medium within young massive…
Infrared Observational Manifestations of Young Dusty Super Star Clusters
Sergio Martinez-Gonzalez, Guillermo Tenorio-Tagle, Sergiy Silich
The growing evidence pointing at core-collapse supernovae as large dust producers makes young massive stellar clusters ideal laboratories to study the evolution of dust immersed in…
On the origin of the absorption and emission line components in the spectra of PHL 293B
Guillermo Tenorio-Tagle, Sergiy Silich, Sergio Martinez-Gonzalez +2
From the structure of PHL 293B and the physical properties of its ionizing cluster and based on results of hydrodynamic models, we point at the various events required to explain i…
On the impact of radiation pressure on the dynamics and inner structure of dusty wind-driven shells
Sergio Martinez-Gonzalez, Sergiy Silich, Guillermo Tenorio-Tagle
Massive young stellar clusters are strong sources of radiation and mechanical energy. Their powerful winds and radiation pressure sweep-up interstellar gas into thin expanding shel…
Young Stellar Clusters with a Schuster Mass Distribution - I: Stationary Winds
Jan Palous, Richard Wunsch, Sergio Martinez-Gonzalez +3
Hydrodynamic models for spherically-symmetric winds driven by young stellar clusters with a generalized Schuster stellar density profile are explored. For this we use both semi-ana…
The Steady State Wind Model for Young Stellar Clusters with an Exponential Stellar Density Distribution
Sergiy Silich, Gennadiy Bisnovatyi-Kogan, Guillermo Tenorio-Tagle +1
A hydrodynamic model for steady state, spherically-symmetric winds driven by young stellar clusters with an exponential stellar density distribution is presented. Unlike in most pr…