ALMA Band 6 high-resolution observations of the transitional disk around SY Chamaeleontis

In this study, we reported the results of high-resolution (0 ''.14) Atacama Large Millimeter/submillimeter Array (ALMA) observations of the 225 GHz dust continuum and CO molecular emission lines from the transitional disk around SY Cha. Our high-resolution observations clearly revealed the inner cavity and the central point source for the first time. The radial profile of the ring can be approximated by a bright narrow ring superimposed on a fainter wide ring. Furthermore, we found that there is a weak azimuthal asymmetry in dust continuum emission. For gas emissions, we detected (CO)-C-12(2-1), (CO)-C-13(2-1), and (CO)-O-18(2-1), from which we estimated the total gas mass of the disk to be 2.2 x 10(-4) M- ?, assuming a CO/H-2 ratio of 10(-4). The observations showed that the gas is present inside the dust cavity. The analysis of the velocity structure of the (CO)-C-12(2-1) emission line revealed that the velocity is distorted at the location of the dust inner disk, which may be owing to a warping of the disk or radial gas flow within the cavity of the dust disk. High-resolution observations of SY Cha showed that this system is composed of a ring and a distorted inner disk, which may be common, as indicated by the survey of transitional disk systems at a resolution of similar to 0 ''.1.