Here is a list of refereed papers either produced within the framework of MaPP, or closely related to the project. Only refereed papers are listed here (small selection for the moment)

Observations & modelling

• 2008 : Donati et al, [http://adsabs.harvard.edu/abs/2008MNRAS.386.1234D Magnetospheric accretion on the T Tauri star BP Tauri]

• 2008 : Jardine et al, [http://adsabs.harvard.edu/abs/2008MNRAS.386..688J Coronal structure of the classical T Tauri star V2129 Oph]

• 2007 : Donati et al, [http://adsabs.harvard.edu/abs/2007MNRAS.380.1297D Magnetic fields and accretion flows on the classical T Tauri star V2129 Oph]

• 2007 : Gregory et al, [http://adsabs.harvard.edu/abs/2007MNRAS.379L..35G Why are accreting T Tauri stars observed to be less luminous in X-rays than non-accretors?]

• 2007 : Johns-Krull, [http://adsabs.harvard.edu/abs/2007ApJ...664..975J The Magnetic Fields of Classical T Tauri Stars]

• 2006 : Gregory et al, [http://adsabs.harvard.edu/abs/2006MNRAS.373..827G Rotationally modulated X-ray emission from T Tauri stars]

• 2006 : Gregory et al, [http://adsabs.harvard.edu/abs/2006MNRAS.371..999G Mass accretion on to T Tauri stars]

• 2006 : Donati et al, [http://adsabs.harvard.edu/abs/2006Sci...311..633D The Large-Scale Axisymmetric Magnetic Topology of a Very-Low-Mass Fully Convective Star]

• 2006 : Jardine et al, [http://adsabs.harvard.edu/abs/2006MNRAS.367..917J X-ray emission from T Tauri stars]

• 2005 : Donati et al, [http://adsabs.harvard.edu/abs/2005Natur.438..466D Direct detection of a magnetic field in the innermost regions of an accretion disk]

Theoretical models & MHD simulations

• 2008 : Long et al, [http://adsabs.harvard.edu/abs/2008MNRAS.386.1274L Three-dimensional simulations of accretion to stars with complex magnetic fields]

• 2008 : Romanova et al, [http://adsabs.harvard.edu/abs/2008ApJ...673L.171R Unstable Disk Accretion onto Magnetized Stars: First Global Three-dimensional Magnetohydrodynamic Simulations]

• 2008 : Commerçon et al, [http://adsabs.harvard.edu/abs/2008A%26A...482..371C Protostellar collapse: a comparison between smoothed particle hydrodynamics and adaptative mesh refinement calculations]

• 2008 : Bessolaz et al, [http://adsabs.harvard.edu/abs/2008A%26A...478..155B Accretion funnels onto weakly magnetized young stars]

• 2008 : Hennebelle & Teyssier, [http://adsabs.harvard.edu/abs/2008A%26A...477...25H Magnetic processes in a collapsing dense core. II. Fragmentation. Is there a fragmentation crisis?]

• 2008 : Hennebelle & Fromang, [http://adsabs.harvard.edu/abs/2008A%26A...477....9H Magnetic processes in a collapsing dense core. I. Accretion and ejection]

In press / submitted / in preparation

• 2008 : Lovelace et al, [http://arxiv.org/abs/0806.4197 Planet Migration and Disk Destruction due to Magneto-Centrifugal Stellar Winds]

• 2008 : Mohanty & Shu, [http://xxx.lanl.gov/abs/0806.4769 Magnetocentrifugally Driven Flows from Young Stars and Disks. VI. Accretion with a Multipole Stellar Field]

• 2008 : Gregory et al, [http://xxx.lanl.gov/abs/0807.0758 The non-dipolar magnetic fields of accreting T Tauri stars]

• 2008 : Hennebelle & Chabrier, [http://arxiv.org/abs/0805.0691 Analytical theory for the initial mass function: CO clumps and prestellar cores]