Hara, C., Kawabe, R., Shimajiri, Y., Ueda, J., Takashi, T., Yasutaka, K., Kazuya, S., Fumitaka, N., Masao, S., and Wilner, David. 2013. "Discovery of the rotating molecular outflow and disk in the Class-0/I protostar [BHB2007]#11 in Pipe." from Astronomical Society of the Pacific Conference Series. 476, 373.
We present the results of our Submillimeter Array (SMA) observations toward a Class-0/I protostar, [BHB2007]#11 (hereafter, B59#11) at the nearby starforming region, Barnard 59 (B59) in the Pipe Nebula (d ˜ 130 pc ; Lombardi et al. 2006) with ˜1″ (corresponding to 130 AU) resolution in CO, 13CO, and C18O(2-1) emissions. We have revealed that a flattened envelope and disk are associated with B59#11. In addition, the outflow ejected from B59#11 might be rotating. We suggest that B59#11 is one of the best targets to reveal the disk/outflow kinematics and address to the angular momentum problem.
