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机译:密集的分子云核是星系中微米级颗粒的来源
Institute of Astronomy and Astrophysics, Academia Sinica, P.O. Box 23-141, Taipei 10617, Taiwan;
Department of Particle and Astrophysical Science, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-8602, Japan;
Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba 277-8583, Japan;
Astronomy Department, University of Virginia, Charlottesville, VA 22904, USA;
Institute of Astronomy and Astrophysics, Academia Sinica, P.O. Box 23-141, Taipei 10617, Taiwan;
Dust; Galaxy evolution; Grain size distribution; Milky Way; Interstellar medium;
机译:Perseus分子云中的致密孔动力学。二。密纹与云之间的关系
机译:巨型分子云Vela C中的密集核和恒星形成
机译:<斜视>赫尔什·斜体>观察Ophiuchus分子云的密集核心群体
机译:在低金属性Dwarf Galaxy WLM中,Alma Co观察揭示了密集的云核心
机译:星系和小麦哲伦星云中分子云的形成
机译:治理云计算与云银河生物医学研究
机译:密集的分子云核心是星系中微米级粒子的来源