Fig. 4 from Imaging the Disk around TW Hydrae with the Submillimeter Array

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Imaging the Disk around TW Hydrae with the Submillimeter Array

Authors: Chunhua Qi, Paul T. P. Ho, David J. Wilner, Shigehisa Takakuwa, Naomi Hirano, Nagayoshi Ohashi, Tyler L. Bourke, Qizhou Zhang, Geoffrey A. Blake, Michiel Hogerheijde, Masao Saito, Minho Choi, and Ji Yang

Qi et al. 2004 The Astrophysical Journal Letters 616 L11.

Provider: AAS Journals

Caption: Fig. 4.

SMA images of the CO ﹩J=3{\mbox{--}} 2﹩ emission from TW Hya in 0.18 km s⁻¹ velocity bins observed with the SMA (upper panels, with a contour spacing of 5 Jy beam⁻¹) together with images from a simulated observation using the model parameters listed in Table 2 (lower panels, with a contour spacing of 3 Jy beam⁻¹). The small cross indicates the position of the continuum source.

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