机译:Dense clumps in giant molecular clouds in the large magellanic cloud: Density and temperature derived from 13CO(J = 3-2) observations
Department of Astrophysics, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-8602, Japan;
Institute of Astronomy, University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-0015, Japan;
Department of Physical Science, Osaka Prefecture University, Gakuen 1-1, Osaka 599-8531 Sakai, JapanInstitute of Science and Technology, Keio University, 4-14-1 Hiyoshi, Kanagawa 223-8522 Yokohama, JapanNational Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588, JapanAstronomy and Space Science Department, Sejong University, 98 Kwangjin-gu, Kunja-dong, Seoul 143-747, South KoreaDepartament de Astronomía, Universidad de Chile, Casilla 36-D, Santiago, ChileDepartment of Physics, Faculty of Science, Hokkaido University, N10W8, Kita-ku, Sapporo 060-0810, JapanDepartment of Cosmosciences, Graduate School of Science, Hokkaido University, N10W8, Kita-ku, Sapporo 060-0810, Japan;
galaxies: individual (LMC); ISM: clouds; ISM: molecules; Magellanic Clouds; radio lines: ISM; submillimeter: general;