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Autor:
Rin I Yamada, Yasuo Fukui, Hidetoshi Sano, Kengo Tachihara, John H Bieging, Rei Enokiya, Atsushi Nishimura, Shinij Fujita, Mikito Kohno, Kisetsu Tsuge
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 515:1012-1025
We have carried out a new kinematical analysis of the molecular gas in the Sh2-233 region by using the CO $J$ = 2-1 data taken at $\sim$0.5 pc resolution. The molecular gas consists of a filamentary cloud of 5-pc length with 1.5-pc width where two de