MaPP|
Size: 1697
Comment:
|
Size: 3398
Comment:
|
| Deletions are marked like this. | Additions are marked like this. |
| Line 1: | Line 1: |
| Only refereed papers are listed here (small selection only for the moment) | #acl MappGroup:read,write All:read |
| Line 3: | Line 3: |
| Here is a list of refereed papers either produced within the framework of MaPP, or closely related to the project. | |
| Line 4: | Line 5: |
| = Observations = | = Observations & modelling = * 2008 : Gregory et al, [http://adsabs.harvard.edu/abs/2008MNRAS.389.1839G The non-dipolar magnetic fields of accreting T Tauri stars] |
| Line 8: | Line 11: |
| * 2008 : Jardine et al, [http://adsabs.harvard.edu/abs/2008MNRAS.386..688J Coronal structure of the classical T Tauri star V2129 Oph] |
|
| Line 9: | Line 14: |
* 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?] |
|
| Line 12: | Line 19: |
| * 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] |
|
| Line 13: | Line 24: |
* 2006 : Jardine et al, [http://adsabs.harvard.edu/abs/2006MNRAS.367..917J X-ray emission from T Tauri stars] |
|
| Line 17: | Line 30: |
| = Simulations = | = Theoretical models & MHD simulations = |
| Line 19: | Line 32: |
| * 2008 : Bessolaz et al, [http://adsabs.harvard.edu/abs/2008A%26A...478..155B Accretion funnels onto weakly magnetized young stars] | * 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] |
| Line 25: | Line 42: |
| * 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] |
|
| Line 28: | Line 49: |
= In press / submitted / in preparation = |
Here is a list of refereed papers either produced within the framework of MaPP, or closely related to the project.
Observations & modelling
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
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]