activity
20112026
most citedMagnetic fields during the early stages of massive star formation - I. Accretion and disk evolution

146 citations · 678 across the 11 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

5 papers · 1 filter

astro-ph.GA2017★ 10 cited

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…

astro-ph.GA2015★ 42 cited

A chemical model for the interstellar medium in galaxies

Stefano Bovino, Tommaso Grassi, Pedro R. Capelo +2

We present and test chemical models for three-dimensional hydrodynamical simulations of galaxies. We explore the effect of changing key parameters such as metallicity, radiation an…

astro-ph.GA2014★ 68 cited

Accretion and magnetic field morphology around Class 0 stage protostellar discs

D. Seifried, R. Banerjee, R. E. Pudritz +1

We analyse simulations of turbulent, magnetised molecular cloud cores focussing on the formation of Class 0 stage protostellar discs and the physical conditions in their surroundin…

astro-ph.GA2013★ 128 cited

Turbulence-induced disc formation in strongly magnetised cloud cores

D. Seifried, R. Banerjee, R. E. Pudritz +1

We present collapse simulations of strongly magnetised, turbulent molecular cloud cores with masses ranging from 2.6 to 1000 M_sun in order to study the influence of the initial co…

astro-ph.GA2012★ 2 cited

Disc formation in turbulent cloud cores: Circumventing the magnetic braking catastrophe

D. Seifried, R. Banerjee, R. E. Pudritz +1

We present collapse simulations of strongly magnetised, 100 M_sun, turbulent cloud cores. Around the protostars formed during the collapse Keplerian discs with typical sizes of up…