activity
20072026
most citedCircumventing the radiation pressure barrier in the formation of massive stars via disk accretion

273 citations · 4.8k across the 100 of their papers we have counts for

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Showing 2020Show all

15 papers · 1 filter

astro-ph.GA2020★ 32 cited

On the compressive nature of turbulence driven by ionising feedback in the pillars of the Carina Nebula

Shyam H. Menon, Christoph Federrath, Pamela Klaassen +2

The ionizing radiation of massive stars sculpts the surrounding neutral gas into pillar-like structures. Direct signatures of star formation through outflows and jets are observed…

astro-ph.SR2020★ 31 cited

Gravity and rotation drag the magnetic field in high-mass star formation

H. Beuther, J. D. Soler, H. Linz +8

The formation of hot stars out of the cold interstellar medium lies at the heart of astrophysical research. Understanding the importance of magnetic fields during star formation re…

astro-ph.GA2020★ 27 cited

Super-Eddington mass growth of intermediate-mass black holes embedded in dusty circumnuclear disks

Daisuke Toyouchi, Kohei Inayoshi, Takashi Hosokawa +1

We perform the first three-dimensional radiation hydrodynamical simulations that investigate the growth of intermediate-mass BHs (IMBHs) embedded in massive self-gravitating, dusty…

astro-ph.IM2020★ 30 cited

Makemake + Sedna: A Continuum Radiation Transport and Photoionization Framework for Astrophysical Newtonian Fluid Dynamics

Rolf Kuiper, Harold W. Yorke, Andrea Mignone

Astrophysical fluid flow studies often encompass a wide range of physical processes to account for the complexity of the system under consideration. In addition to gravity, a prope…

astro-ph.SR2020★ 32 cited

Photoevaporation of Grain-Depleted Protoplanetary Disks around Intermediate-Mass Stars: Investigating Possibility of Gas-Rich Debris Disks as Protoplanetary Remnants

Riouhei Nakatani, Hiroshi Kobayashi, Rolf Kuiper +2

Debris disks are classically considered to be gas-less systems, but recent (sub)millimeter observations have detected tens of those with rich gas content. The origin of the gas com…

astro-ph.SR2020★ 70 cited

Modeling disk fragmentation and multiplicity in massive star formation

G. André Oliva, Rolf Kuiper

We investigate the formation and early evolution and fragmentation of an accretion disk around a forming massive protostar. We use a grid-based self-gravity-radiation-hydrodynamics…