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- W2154756980 abstract "We present a method that uses disk models to determine stellar masses for Pre-Main sequence T Tauri stars from JHK photometry. We nd that the infrared excess produced by the disk behaves in a similar way to the extinction vector when plotted on color-color and color-magnitude diagrams, but that it is linearly independent. Employing these vectors as a basis of a vector space we carry out a coordinate transformation that allows us to nd the mass of a central star for a given age. To test this Principal Vectors (PV) method we compare the mass values (MP V ) obtained for 14 T Tauri objects in the Taurus-Auriga region with mass values known from dynamical methods. Furthermore, we analyze 4 systems with multiple components (GG Tau, FO Tau, FS Tau, and V773 Tau) and determine the mass for each component of the system. We analyze the eect of using dieren t evolutionary models and other parameter values." @default.
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- W2154756980 date "2007-04-01" @default.
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- W2154756980 title "Mass Determination for T Tauri Stars from JHK Photometry" @default.
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