367 citations · 2.7k across the 54 of their papers we have counts for
54 papers
X-rays from shock-heated gas in recurrent-nova remnants: Nested nova shells in a structured circumstellar medium
Sergio Martínez-González, Santiago Jiménez, Richard Wünsch +1
Recurrent symbiotic novae such as RS Oph show extended X-ray emission associated with the interaction of nova ejecta with the circumstellar environment. We investigate how repeated…
Bipolar HII regions Produced by Cloud-Cloud Collisions
Theotokis Georgatos, Anthony P. Whitworth, Richard Wünsch +1
We use numerical experiments to explore two possibilities: (i) that Bipolar H II Regions are the result of Cloud-Cloud Collisions (CCCs), and (ii) that -- when allowance is made fo…
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…
The bright, dusty aftermath of giant eruptions & H-rich supernovae. Late interaction of supernova shocks & dusty circumstellar shells
Diana B. Serrano-Hernández, Sergio Martínez-González, Santiago Jiménez +2
The late-stage evolution of massive stars is marked by intense instability as they approach core-collapse. During these phases, giant stellar eruptions lead to exceptionally high m…
Radiation transport methods in star formation simulations
Richard Wünsch
Radiation transport plays a crucial role in star formation models, as certain questions within this field cannot be accurately addressed without taking it into account. Given the h…
Ionized regions in the central arcsecond of NGC 1068. YJHK spatially resolved spectroscopy
P. Vermot, B. Barna, S. Ehlerová +3
Context. Several bright emission line regions have been observed in the central 100 parsecs of the active galaxy NGC 1068. Aims. We aim to determine the properties and ionization m…