39 citations · 154 across the 11 of their papers we have counts for
11 papers
Synthetic observations using POLARIS: an application to simulations of massive prestellar cores
Joaquin Zamponi, Andrea Giannetti, Stefano Bovino +5
Young massive stars are usually found embedded in dense and massive molecular clumps which are known for being highly obscured and distant. During their formation process, the degr…
The relative orientation between the magnetic field and gas density structures in non-gravitating turbulent media
Bastian Körtgen, Juan D. Soler
Magnetic fields are a dynamically important agent for regulating structure formation in the interstellar medium. The study of the relative orientation between the local magnetic fi…
Synthetic observations of deuterated molecules in massive prestellar cores
Joaquin Zamponi F., Andrea Giannetti, Stefano Bovino +5
Young massive stars are usually found embedded in dense massive molecular clumps and are known for being highly obscured and distant. During their formation process, deuteration is…
Structure and Expansion Law of HII Regions in structured Molecular Clouds
Manuel Zamora-Avilés, Enrique Vázquez-Semadeni, Ricardo F. González +6
We present radiation-magnetohydrodynamic simulations aimed at studying evolutionary properties of H\,{\normalsize II} regions in turbulent, magnetised, and collapsing molecular clo…
The Origin of Filamentary Star Forming Clouds in Magnetised Galaxies
Bastian Körtgen, Robi Banerjee, Ralph E. Pudritz +1
Observations show that galaxies and their interstellar media are pervaded by strong magnetic fields with energies in the diffuse component being at least comparable to the thermal…
Star formation in evolving molecular clouds
M. Völschow, R. Banerjee, B. Körtgen
Molecular clouds are the principle stellar nurseries of our universe, keeping them in the focus of both observational and theoretical studies. From observations, some of the key pr…
The driving of turbulence in simulations of molecular cloud formation and evolution
Bastian Körtgen, Christoph Federrath, Robi Banerjee
Molecular clouds are to a great extent influenced by turbulent motions in the gas. Numerical and observational studies indicate that the star formation rate and efficiency cruciall…
Deuterium fractionation and H2D+ evolution in turbulent and magnetized cloud cores
Bastian Körtgen, Stefano Bovino, Dominik R. G. Schleicher +2
High-mass stars are expected to form from dense prestellar cores. Their precise formation conditions are widely discussed, including their virial condition, which results in slow c…
Formation of star-forming clouds from the magnetised, diffuse interstellar medium
Robi Banerjee, Bastian Körtgen
Molecular clouds, the birthplaces of stars in galaxies, form dynamically from the diffuse atomic gas of the interstellar medium (ISM). The ISM is also threaded by magnetic fields w…
Tracing the general structure of Galactic molecular clouds using Planck data: I. The Perseus region as a test case
Orlin Stanchev, Todor V. Veltchev, Jens Kauffmann +4
We present an analysis of probability distribution functions (pdfs) of column density in different zones of the star-forming region Perseus and its diffuse environment based on the…
Impact Of Magnetic Fields On Molecular Cloud Formation & Evolution
Bastian Körtgen, Robi Banerjee
We use magnetohydrodynamical simulations of converging flows to investigate the process of molecular cloud formation and evolution out of the magnetised ISM. Here, we investigate w…