Figure 3 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 3.

Extinction-corrected U–R color–magnitude diagram of emission above the stellar photosphere. Encircled points highlight candidate flares from high-cadence light-curve analysis. The bluest point observed in U–R is the peak emission of “Flare 1” presented in Figure 5 (see text). (Extinction and template determination are discussed in Section 4.)

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