Fig. 1 from Chandra and ASCA Observations of the X‐Ray–brightest T Tauri Stars in the ρ Ophiuchi Cloud

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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. 1.

Light curves of (a) DoAr 21, (b) ROXs 21, and (c) ROXs 31 in 0.5–9.0 keV, obtained with Chandra ACIS (observation C1). The vertical axis is the X‐ray count rate normalized in the effective area of 100 cm² at 1 keV. The bottom arrows indicate the times of the flare and quiescent phases (see Table 2).

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