MaPPHere is a list of refereed papers either produced within the framework of MaPP, or closely related to the project.
Observations & modelling
2010 : Donati et al, [http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1007.4407 Magnetospheric accretion and spin-down of the prototypical classical T Tauri star AATau]
2010 : Skelly et al, [http://adsabs.harvard.edu/abs/2010MNRAS.403..159S Dynamo processes in the T Tauri star V410 Tau]
2010 : Donati et al, [http://adsabs.harvard.edu/abs/2010MNRAS.402.1426D Complex magnetic topology and strong differential rotation on the low-mass T Tauri star V2247 Oph]
2009 : Donati & Landstreet, [http://adsabs.harvard.edu/abs/2009ARA%26A..47..333D Magnetic Fields of Nondegenerate Stars]
2009 : Hussain et al, [http://adsabs.harvard.edu/abs/2009MNRAS.398..189H Surface magnetic fields on two accreting TTauri stars: CVCha and CRCha]
2008 : Gregory et al, [http://adsabs.harvard.edu/abs/2008MNRAS.389.1839G The non-dipolar magnetic fields of accreting T Tauri stars]
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
2010 : Gregory et al, [http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1008.1883 The magnetic fields of forming solar-like stars]
2009 : Hennebelle et al, [http://adsabs.harvard.edu/abs/2009A%26A...506L..29H Disk formation during collapse of magnetized protostellar cores]
2008 : Lovelace et al, [http://adsabs.harvard.edu/abs/2008MNRAS.389.1233L Planet Migration and Disk Destruction due to Magneto-Centrifugal Stellar Winds]
2008 : Hennebelle & Chabrier, [http://adsabs.harvard.edu/abs/2008ApJ...684..395H Analytical theory for the initial mass function: CO clumps and prestellar cores]
2008 : Mohanty & Shu, [http://adsabs.harvard.edu/abs/2008ApJ...687.1323M Magnetocentrifugally Driven Flows from Young Stars and Disks. VI. Accretion with a Multipole Stellar Field]
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]