Locked History Attachments

MAPP: Diff for "MappPapers"

Differences between revisions 1 and 7 (spanning 6 versions)
Revision 1 as of 2008-07-02 16:00:40
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Revision 7 as of 2008-07-10 15:18:00
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#acl MappGroup:read,write All:read
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= Observations = = Observations & modelling =
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 * 2008 : Jardine et al, [http://adsabs.harvard.edu/abs/2008MNRAS.386..688J Coronal structure of the classical T Tauri star V2129 Oph]
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 * 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?]
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 * 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]
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 * 2006 : Jardine et al, [http://adsabs.harvard.edu/abs/2006MNRAS.367..917J X-ray emission from T Tauri stars]
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= Simulations = = Theoretical models & MHD simulations =
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= In press / submitted / in preparation =

 * 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]

Only refereed papers are listed here (small selection only for the moment)

Observations & modelling

Theoretical models & MHD simulations

In press / submitted / in preparation