Figure 10 from ACCRETION AND MAGNETIC RECONNECTION IN THE CLASSICAL T TAURI BINARY DQ TAU

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ACCRETION AND MAGNETIC RECONNECTION IN THE CLASSICAL T TAURI BINARY DQ TAU

Authors: Benjamin M. Tofflemire, Robert D. Mathieu, David R. Ardila, Rachel L. Akeson, David R. Ciardi, Christopher Johns-Krull, Gregory J. Herczeg, and Alberto Quijano-Vodniza

2017 The Astrophysical Journal 835 8.

Provider: AAS Journals

Caption: Figure 10.

The mass accretion rate (left axis) of the most active and most passive orbital periods. The green and black data are from orbital cycles 2 and 4, respectively. The blue histogram is orbit-averaged accretion rate from Figure 8. The right axis presents the corresponding accretion luminosity.

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