Figure 11 from ACCRETION AND MAGNETIC RECONNECTION IN THE CLASSICAL T TAURI BINARY DQ TAU

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 11.

U–B color of the excess accretion luminosity vs. the U-band excess above the stellar photosphere (flares removed). The U-band excess luminosity is a proxy for the mass accretion rate. A variety of U − B excess colors are present for given U-band excess.

Other Images in This Article

Copyright and Terms & Conditions