Akiharu Nakagawa, Miyuki Tsushima, Kazuma Ando, Takeshi Bushimata, Yoon Kyung Choi, Tomoya Hirota, Mareki Honma, Hiroshi Imai, Kenzaburo Iwadate, Takaaki Jike, Seiji Kameno, Osamu Kameya, Ryuichi Kamohara, Yukitoshi Kan-ya, Noriyuki Kawaguchi, Masachika Kijima, Mi Kyoung Kim, Hideyuki Kobayashi, Seisuke Kuji, Tomoharu Kurayama, Toshihisa Maeda, Seiji Manabe, Kenta Maruyama, Makoto Matsui, Naoko Matsumoto, Takeshi Miyaji, Takumi Nagayama, Kayoko Nakamura, Daisuke Nyu, Chung Sik Oh, Toshihiro Omodaka, Tomoaki Oyama, Nicolas Pradel, Satoshi Sakai, Tetsuo Sasao, Katsuhisa Sato, Mayumi Sato, Katsunori M. Shibata, Hiroshi Suda, Yoshiaki Tamura, Kousuke Ueda, Yuji Ueno, Kazuyoshi Yamashita
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 60(5) 1013-1021 2008年10月
We present a distance measurement for the semiregular variable S Crateris (S Crt) based on its annual parallax. With the unique dual beam system of the VLBI Exploration for Radio Astrometry (VERA) telescopes, we measured the absolute proper motion of a water maser spot associated with S Crt, referred to the quasar J1147-0724 located at an angular separation of 1.degrees 23. In observations spanning nearly two years, we detected the maser spot at an LSR velocity of 34.7 km s(-1), for which we measured an annual parallax of 2.33 +/- 0.13 mas, corresponding to a distance of 430(-23)(+25) pc. This measurement has an accuracy one order of magnitude better than the parallax measurements of HIPPARCOS. The angular distribution and three-dimensional velocity fieI6 of maser spots indicate a bipolar outflow with the flow axis along the northeast-south west direction. Using the distance and photospheric temperature, we estimated the stellar radius of S Crt and compared it with those of Mira variables.