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Chandra and ASCA Observations of the X‐Ray–brightest T Tauri Stars in the ρ Ophiuchi Cloud

  • Authors: Kensuke Imanishi, Masahiro Tsujimoto, and Katsuji Koyama

Imanishi, Tsujimoto, & Koyama 2002 The Astrophysical Journal 572 300.

  • Provider: AAS Journals

Caption: Fig. 5.

Close‐up view of the fitting results of ROXs 21 in phase Q, in which (a) Na abundance is varied correctively with the "other" elements and (b) is treated as a free parameter. The positions of K‐shell lines from (a) Ne and (b) Na are shown by arrows. The prominent feature near the Lyα line of Na is also indicated by dashed rectangles.

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