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T Tauri stars : mass accretion and X ray emission

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Figure

Figure 1.1: An idealised model of the magnetic field structure of a classical T
Figure 1.2: The SED of the CTTs BP Tau. The dashed line is the SED we
Figure 1.3: The correlations between mass accretion rate and CaII emission line
Figure 1.4: Sections of the spectrum of BP Tau, reproduced from Johns-Krull
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