Figure 8 from Near-ultraviolet Excess in Slowly Accreting T Tauri Stars: Limits Imposed by Chromospheric Emission

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Near-ultraviolet Excess in Slowly Accreting T Tauri Stars: Limits Imposed by Chromospheric Emission

Authors: Laura Ingleby, Nuria Calvet, Edwin Bergin, Gregory Herczeg, Alexander Brown, Richard Alexander, Suzan Edwards, Catherine Espaillat, Kevin France, Scott G. Gregory, Lynne Hillenbrand, Evelyne Roueff, Jeff Valenti, Frederick Walter, Christopher Johns-Krull, Joanna Brown, Jeffrey Linsky, Melissa McClure, David Ardila, Hervé Abgrall, Thomas Bethell, Gaitee Hussain, and Hao Yang

Ingleby et al. 2011 The Astrophysical Journal 743 105.

Provider: AAS Journals

Caption: Figure 8.

STIS spectrum of RECX-11 compared to predictions of the accretion shock model. Top panel: we show the STIS spectrum of RECX-11 (thin solid line) along with the template NUV and optical emission, the WTTS RECX-1 (red dotted line), and the emission predicted from the accretion shock model (blue long dashed line), with . The thick solid green spectrum is the accretion shock model added to the WTTS spectrum. Bottom panel: the model (green) was subtracted from the observations (black) and the residuals are shown.

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