Figure 5 from Panchromatic Observations and Modeling of the HV Tau C Edge-on Disk

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Panchromatic Observations and Modeling of the HV Tau C Edge-on Disk

Authors: G. Duchêne, C. McCabe, C. Pinte, K. R. Stapelfeldt, F. Ménard, G. Duvert, A. M. Ghez, H. L. Maness, H. Bouy, D. Barrado y Navascués, M. Morales-Calderón, S. Wolf, D. L. Padgett, T. Y. Brooke, and A. Noriega-Crespo

DUCHÊNE et al. 2010 The Astrophysical Journal 712 112.

Provider: AAS Journals

Caption: Figure 5.

PdBI 1.3 mm correlated fluxes for HV Tau C as a function of projected baseline length for all baselines that are within 22 fdg 5 of the disk major axis (squares) and within 22 fdg 5 of its minor axis (diamonds). The major axis is assumed to be 108 fdg 3 as determined from the scattered light images. The dashed and dotted curves represent the major- and minor-axis of the Gaussian fit to all visibilities, respectively, assuming a Gaussian 0 farcs 3 atmospheric "seeing."

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