Rolf Kuiper

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Universität Duisburg-Essen

Germany

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Rolf Kuiper is a Professor at the University of Duisburg-Essen, Germany. His research areas include high-mass star formation, accretion processes, and the evolution of protoplanetary disks, as evidenced by his recent articles on thermal instability and black hole growth. With a focus on both theoretical models and simulations, he explores the fundamental processes that govern stellar and planetary evolution.

Recent Grants

Grant: Close

BLOBS: Birth and Life of OB Stars

Open Date: 2021-01-01

Close Date:

Grant: Close

Formation and early evolution of gas giants: Shocks and planetary spins

Open Date: 2020-01-01

Close Date:

Grant: Close

NLTE in the upper atmospheres of exoplanets

Open Date: 2020-01-01

Close Date:

Grant: Close

The Formation of Planetary Proto-Atmospheres

Open Date: 2017-01-01

Close Date:

Grant: Close

Formation and early evolution of gas giants: The accretion shock and its consequences

Open Date: 2017-01-01

Close Date:

Rolf Kuiper

Research Interests

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Recent Grants

Articles (24)

Episodic accretion in high-mass star formation: An analysis of thermal instability for axially symmetric disks

X-Shooting ULLYSES: Massive stars at low metallicity

Testing the bloated star hypothesis in the massive young stellar object IRAS 19520+2759 through optical and infrared variability

Physically motivated analytic model of energy efficiency for extreme-ultraviolet-driven atmospheric escape of close-in exoplanets

Impact of accretor size on the morphology of supersonic, non-relativistic, axisymmetric Bondi-Hoyle-Lyttleton accretion flows

Radiation hydrodynamical simulations of super-Eddington mass transfer and black hole growth in close binaries

Mixing is easy: New insights for cosmochemical evolution from pre-stellar core collapse

The Effect of Ultraviolet Photon Pumping of H2 in Dust-deficient Protoplanetary Disks

Observations of high-order multiplicity in a high-mass stellar protocluster

A probable Keplerian disk feeding an optically revealed massive young star

The role of thermal instability in accretion outbursts in high-mass stars

Two-dimensional simulations of disks in close binaries

The Planetary Accretion Shock. III. Smoothing-free 2.5D Simulations and Calculation of Hα Emission

Atmospheric recycling of volatiles by pebble-accreting planets

Disk fragmentation around a massive protostar: Comparison of two 3D codes

Kinematics and stability of high-mass protostellar disk candidates at sub-arcsecond resolution

Radiative feedback on supermassive star formation: the massive end of the Population III initial mass function

Long-term Evolution of Supercritical Black Hole Accretion with Outflows: A Subgrid Feedback Model for Cosmological Simulations

Supercritical Growth Pathway to Overmassive Black Holes at Cosmic Dawn: Coevolution with Massive Quasar Hosts

VETTAM: a scheme for radiation hydrodynamics with adaptive mesh refinement using the variable Eddington tensor method

Rapid Growth of Seed Black Holes during Early Bulge Formation

Snapshot of a magnetohydrodynamic disk wind traced with water masers

Discovery of Molecular-line Polarization in the Disk of TW Hya

Stability of an ionization front in Bondi accretion

Collaborators (15)

Qizhou Zhang

Paul Crowther

Gabriel-Dominique Marleau

Kotomi Taniguchi

Stuart Lumsden

Fernando Olguin Choupay

Thomas Möller

Riouhei Nakatani

ANDREA MIGNONE

Ralph Pudritz

Manuel Jung

Charles Hull

Matthias González

Anna Faye McLeod

Shanghuo Li

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