机译:ALMA观察Z的富含气体的星系类似于1.6个星系集群:高密度环境中较高气体级分的证据
MIT Kavli Inst Astrophys &
Space Res 77 Massachusetts Ave Cambridge MA 02139 USA;
MIT Kavli Inst Astrophys &
Space Res 77 Massachusetts Ave Cambridge MA 02139 USA;
York Univ Dept Phys &
Astron 4700 Keele St Toronto ON MJ3 1P3 Canada;
Univ Andres Bello Dept Ciencias Fis Fernandez Concha 700 Santiago 7591538 Regiin Metropol Chile;
Univ Kansas Dept Phys &
Astron 1251 Wescoe Hall Dr Lawrence KS 66045 USA;
European Southern Observ Karl Schwarzschild Str 2 D-85748 Garching Germany;
McGill Univ Dept Phys 3600 Rue Univ Montreal PQ H3A 2T8 Canada;
Univ Calif Riverside Dept Phys &
Astron Riverside CA 92521 USA;
Univ Toronto Dept Astron &
Astrophys 50 St George St Toronto ON M5S 3H4 Canada;
Univ Calif Berkeley Dept Phys 366 LeConte Hall MC 7300 Berkeley CA 94720 USA;
Univ Calif Irvine Dept Phys &
Astron 4129 Frederick Reines Hall Irvine CA 92697 USA;
Univ Calif Riverside Dept Phys &
Astron Riverside CA 92521 USA;
McGill Univ Dept Phys 3600 Rue Univ Montreal PQ H3A 2T8 Canada;
Univ Concepcion Dept Astron Casilla 160-C Concepcion Region Del Biob Chile;
Univ Calif Riverside Dept Phys &
Astron Riverside CA 92521 USA;
Univ Calif Berkeley Dept Phys 366 LeConte Hall MC 7300 Berkeley CA 94720 USA;
Australian Astron Observ 105 Delhi Rd N Ryde NSW 2113 Australia;
European Southern Observ Karl Schwarzschild Str 2 D-85748 Garching Germany;
Univ Calif Berkeley Dept Phys 366 LeConte Hall MC 7300 Berkeley CA 94720 USA;
galaxies: clusters: general; galaxies: evolution; galaxies: high-redshift; galaxies: ISM; galaxies: star formation; infrared: galaxies;
机译:ALMA观察Z的富含气体的星系类似于1.6个星系集群:高密度环境中较高气体级分的证据
机译:z = 1-1.5时的簇和场星系活动银河系核分数:环境与Agn分数之间的局部反相关的证据
机译:z = 4.05时分子富集星系的原始聚类的扩展超大型阵列观测
机译:天线银河碰撞的alma视图:星系交互如何触发超级星团的形成
机译:银河系中的结构与环境在模拟与观察中
机译:无线电源星系和星系群
机译:aL~1~1银河系中富含气体的星系的aLma观测:高密度环境中高气体分数的证据