Papers

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2010 Romain Teyssier

, Damien Chapon, Frédéric Bournaud

The Driving Mechanism of Starbursts in Galaxy Mergers

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Miguel Pato, Oscar Agertz, Gianfranco Bertone, Ben Moore, Romain Teyssier

Systematic uncertainties in the determination of the local dark matter density

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Frédéric Bournaud, Leila C. Powell, Damien Chapon, Romain Teyssier

Star formation in galaxy mergers: ISM turbulence, dense gas excess, and scaling relations for disks and starbusts

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Oliver Hahn, Romain Teyssier

, C. Marcella Carollo

The large-scale orientations of disc galaxies

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Leila C. Powell, Frederic Bournaud, Damien Chapon, Julien Devriendt, Adrianne Slyz, Romain Teyssier

Galactic star formation in parsec-scale resolution simulations

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Benoît Commerçon

, Patrick Hennebelle, Edouard Audit, Gilles Chabrier, Romain Teyssier

Radiative, magnetic and numerical feedbacks on small-scale fragmentation

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Romain Teyssier, Ben Moore, Davide Martizzi

, Yohan Dubois, Lucio Mayer

Mass Distribution in Galaxy Clusters: the Role of AGN Feedback

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2009 Marie Martig

, Frédéric Bournaud, Romain Teyssier

, Avishai Dekel

Morphological Quenching of Star Formation: Making Early-Type Galaxies Red

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Aaron C. Boley, George Lake, Justin Read, Romain Teyssier

Globular Cluster Formation Within a Cosmological Context

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Oscar Agertz, Romain Teyssier

, Ben Moore

Disc formation and the origin of clumpy galaxies at high redshift

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Oscar Agertz, George Lake, Romain Teyssier

, Ben Moore, Lucio Mayer, Alessandro B. Romeo

Large-scale galactic turbulence: can self-gravity drive the observed H i velocity dispersions?

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2008 Marie Martig, Frédéric Bournaud, Romain Teyssier

Numerical simulations of galaxy evolution in cosmological context

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Dominique Aubert, Romain Teyssier

A radiative transfer scheme for cosmological reionization based on a local Eddington tensor

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Brad K. Gibson

, Stéphanie Courty, Patricia Sánchez-Blázquez, Romain Teyssier

, Elisa L. House, Chris B. Brook, Daisuke Kawata

Hydrodynamical Adaptive Mesh Refinement Simulations of Disk Galaxies

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2007 Oscar Agertz, Ben Moore, Joachim Stadel, Doug Potter, Francesco Miniati, Justin Read, Lucio Mayer, Artur Gawryszczak, Andrey Kravtsov, Åke Nordlund, Frazer Pearce, Vicent Quilis, Douglas Rudd, Volker Springel

, James Stone and 4 other authors

Fundamental differences between SPH and grid methods

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Daniel Pomarède, Edouard Audit, Romain Teyssier

, Bruno Thooris

Visualization of large astrophysical simulations datasets

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Romain Teyssier

A high order Godunov scheme with constrained transport and adaptive mesh refinement for astrophysical and geophysical MHD

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2006 Romain Teyssier

, Sébastien Fromang, Emmanuel Dormy

Kinematic dynamos using constrained transport with high order Godunov schemes and adaptive mesh refinement

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Yann Rasera, Romain Teyssier

, Patrick Sizun, Michel Cassé, Pierre Fayet, Bertrand Cordier, Jacques Paul

Soft gamma-ray background and light dark matter annihilation

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Olivier Doré, François R. Bouchet, Romain Teyssier, Didier Vibert

CMB Data Analysis: the Map-Making Problem

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