UB Paderborn / Katalog / Suche / in CDI

The chemistry of protoplanetary fragments formed via gravitational instabilities

Monthly notices of the Royal Astronomical Society, 2017-11, Vol.472 (1), p.189-204

2017

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Star Formation Around Supermassive Black Holes

Science (American Association for the Advancement of Science), 2008-08, Vol.321 (5892), p.1060-1062

2008

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Particle acceleration and coronal mass ejection driven shocks: A theoretical model

Journal of Geophysical Research, 2000-11, Vol.105 (A11), p.25079-25095

2000

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Dust filtration at gap edges: implications for the spectral energy distributions of discs with embedded planets

Monthly notices of the Royal Astronomical Society, 2006-12, Vol.373 (4), p.1619-1626

2006

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Time-dependent models of the structure and stability of self-gravitating protoplanetary discs

Monthly notices of the Royal Astronomical Society, 2009-07, Vol.396 (4), p.2228-2236

2009

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Have protoplanetary discs formed planets?

Monthly notices of the Royal Astronomical Society, 2010-09, Vol.407 (3), p.1981-1988

2010

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Testing the locality of transport in self-gravitating accretion discs — II. The massive disc case

Monthly notices of the Royal Astronomical Society, 2005-04, Vol.358 (4), p.1489-1500

2005

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The role of disc self-gravity in the formation of protostars and protostellar discs

Monthly notices of the Royal Astronomical Society, 2010-03, Vol.402 (3), p.1740-1749

2010

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Convergence of simulations of self-gravitating accretion discs – II. Sensitivity to the implementation of radiative cooling and artificial viscosity

Monthly notices of the Royal Astronomical Society, 2014-02, Vol.438 (2), p.1593-1602

2014

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Planetesimal formation in self-gravitating discs – dust trapping by vortices

Monthly notices of the Royal Astronomical Society, 2015-11, Vol.453 (4), p.4232-4243

2015

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Planetesimal formation in self-gravitating discs – the effects of particle self-gravity and back-reaction

Monthly notices of the Royal Astronomical Society, 2014-07, Vol.442 (1), p.361-371

2014

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Misaligned streamers around a Galactic Centre black hole from a single cloud's infall

Monthly notices of the Royal Astronomical Society, 2013, Vol.433 (1), p.353-365

2013

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Accelerated planetesimal growth in self-gravitating protoplanetary discs

Monthly notices of the Royal Astronomical Society, 2004-12, Vol.355 (2), p.543-552

2004

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Acceleration and transport of heavy ions at coronal mass ejection-driven shocks

Journal of Geophysical Research - Space Physics, 2005-06, Vol.110 (A6), p.A06104-n/a

2005

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Axisymmetric modes in vertically stratified self-gravitating discs

Monthly notices of the Royal Astronomical Society, 2010-08, Vol.406 (3), p.2050-2064

2010

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Towards a population synthesis model of self-gravitating disc fragmentation and tidal downsizing II: the effect of fragment–fragment interactions

Monthly notices of the Royal Astronomical Society, 2018-03, Vol.474 (4), p.5036-5048

2018

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The effect of cooling on the global stability of self-gravitating protoplanetary discs

Monthly notices of the Royal Astronomical Society, 2003-03, Vol.339 (4), p.1025-1030

2003

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Vortices in self-gravitating gaseous discs

Monthly notices of the Royal Astronomical Society, 2009-04, Vol.394 (4), p.2153-2163

2009

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Why are there so few hot Jupiters?

Monthly notices of the Royal Astronomical Society, 2008-03, Vol.384 (3), p.1242-1248

2008

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Testing the locality of transport in self-gravitating accretion discs

Monthly notices of the Royal Astronomical Society, 2004-06, Vol.351 (2), p.630-642

2004

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On the Formation Timescale and Core Masses of Gas Giant Planets

The Astrophysical journal, 2003-11, Vol.598 (1), p.L55-L58

2003

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The role of the energy equation in the fragmentation of protostellar discs during stellar encounters

Monthly notices of the Royal Astronomical Society, 2007-01, Vol.374 (2), p.590-598

2007

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Planetesimal formation in self‐gravitating discs

Monthly notices of the Royal Astronomical Society, 2012-10, Vol.426 (2), p.1444-1454

2012

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Stability of self-gravitating discs under irradiation

Monthly notices of the Royal Astronomical Society, 2011-12, Vol.418 (2), p.1356-1362

2011

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Convergence of smoothed particle hydrodynamics simulations of self-gravitating accretion discs: sensitivity to the implementation of radiative cooling

Monthly notices of the Royal Astronomical Society, 2012-02, Vol.420 (2), p.1640-1647

2012

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The chemistry of protoplanetary fragments formed via gravitational instabilities

Star Formation Around Supermassive Black Holes

Particle acceleration and coronal mass ejection driven shocks: A theoretical model

Dust filtration at gap edges: implications for the spectral energy distributions of discs with embedded planets

Time-dependent models of the structure and stability of self-gravitating protoplanetary discs

Have protoplanetary discs formed planets?

Testing the locality of transport in self-gravitating accretion discs — II. The massive disc case

The role of disc self-gravity in the formation of protostars and protostellar discs

Convergence of simulations of self-gravitating accretion discs – II. Sensitivity to the implementation of radiative cooling and artificial viscosity

Planetesimal formation in self-gravitating discs – dust trapping by vortices

Planetesimal formation in self-gravitating discs – the effects of particle self-gravity and back-reaction

Misaligned streamers around a Galactic Centre black hole from a single cloud's infall

Accelerated planetesimal growth in self-gravitating protoplanetary discs

Acceleration and transport of heavy ions at coronal mass ejection-driven shocks

Axisymmetric modes in vertically stratified self-gravitating discs

Towards a population synthesis model of self-gravitating disc fragmentation and tidal downsizing II: the effect of fragment–fragment interactions

The effect of cooling on the global stability of self-gravitating protoplanetary discs

Vortices in self-gravitating gaseous discs

Why are there so few hot Jupiters?

Testing the locality of transport in self-gravitating accretion discs

On the Formation Timescale and Core Masses of Gas Giant Planets

The role of the energy equation in the fragmentation of protostellar discs during stellar encounters

Planetesimal formation in self‐gravitating discs

Stability of self-gravitating discs under irradiation

Convergence of smoothed particle hydrodynamics simulations of self-gravitating accretion discs: sensitivity to the implementation of radiative cooling

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