机译:爆发星系的堆叠星形成速率概况表现出“相干”的星形形成
TAPIR Mailcode 350-17 California Institute of Technology Pasadena CA 91125 USA;
Center for Computational Astrophysics Flatiron Institute 162 Fifth Avenue New York NY 10010 USA;
Max-Planck-Institut für Extraterrestriche Physik Giessenbachstrasse D-85748 Garching Germany;
TAPIR Mailcode 350-17 California Institute of Technology Pasadena CA 91125 USA;
Department of Physics and Astronomy and CIERA Northwestern University 2145 Sheridan Road Evanston IL 60208 USA;
Department of Physics Center for Astrophysics and Space Science University of California San Diego 9500 Gilman Drive La Jolla CA 92093 USA;
Department of Physics Center for Astrophysics and Space Science University of California San Diego 9500 Gilman Drive La Jolla CA 92093 USA;
TAPIR Mailcode 350-17 California Institute of Technology Pasadena CA 91125 USA;
Department of Astronomy Yale University 52 Hillhouse Avenue New Haven CT 06511 USA;
galaxies: evolution; galaxies: formation; galaxies: high-redshift; galaxies: star formation; galaxies: structure; methods: observational;
机译:爆发星系的堆叠星形成速率概况表现出“相干”的星形形成
机译:邻近螺旋星系中的特定恒星形成速率曲线:量化盘的由内而外的形成
机译:邻近旋涡星系中特定恒星形成速率的分布图:量化盘的内外形成
机译:Z〜2的分子气,恒星和灰尘的新出现结果,如低星形形成速率和低恒星大规模星形星系所揭示的
机译:恒星形成星系的形态学特征:将过去90亿年中星系的形态演变与宇宙恒星形成率密度的下降联系起来。
机译:镜头GALAXY SDSS J1110 + 6459中Z = 2.481时的恒星形成:低至30帕斯卡尺度的恒星形成
机译:爆发星系的堆叠星形成速率概况表现出“相干”的星形形成