机译:气流穿过原行星间隙
Departamento de Astronomia, Universidad de Chile, Casilla 36-D, Santiago, Chile;
Departamento de Astronomia, Universidad de Chile, Casilla 36-D, Santiago, Chile;
Departamento de Astronomia, Universidad de Chile, Casilla 36-D, Santiago, Chile;
Joint ALMA Observatory, Alonso de Cordova 3107, Vitacura 763-0355, Santiago, Chile,European Southern Observatory, Casilla 19001, Vitacura, Santiago, Chile;
National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, Virginia 22903-2475, USA;
Observatoire de Geneve, Universite de Geneve, 51 Chemin des Maillettes, 1290, Versoix, Switzerland;
Joint ALMA Observatory, Alonso de Cordova 3107, Vitacura 763-0355, Santiago, Chile,National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, Virginia 22903-2475, USA;
Departamento de Astronomia y Astrofisica, Pontificia Universidad Catolica de Chile, Santiago, Chile;
European Southern Observatory, Casilla 19001, Vitacura, Santiago, Chile;
UMI-FCA, CNRS/INSU France (UMI 3386), and Departamento de Astronomia, Universidad deChile,Santiago,Chile,CNRS/UJFGrenoblel,UMR 5274, lnstitutdePlanetologieetdAstrophysiquedeGrenoble(IPAG),F-48041GrenobleCedex 9, France;
National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, Virginia 22903-2475, USA;
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138, USA;
Department of Astronomy, UC Berkeley, 601 Campbell Hall, Berkeley, California 94720, USA;
Departamento de Fisica y Astronomia, Universidad Valparaiso, Avenida Gran Bretana 1111, Valparaiso, Chile;
European Southern Observatory, Casilla 19001, Vitacura, Santiago, Chile;
University Observatory, Ludwig-Maximillians University, D-81679 Munich,Germany;
Departamento de Fisica y Astronomia, Universidad Valparaiso, Avenida Gran Bretana 1111, Valparaiso, Chile;
Center of Mathematical Modeling, University of Chile, Avenida Blanco Encalada 2120 Piso 7, Santiago, Chile;
Departamento de Astronomia, Universidad de Chile, Casilla 36-D, Santiago, Chile;
机译:多环芳烃离子化作为气体的示踪剂流过原行星盘间隙
机译:原始盘中气体跨间隙的流动
机译:原始盘中气体在整个间隙中的流动
机译:3D原始磁盘灰尘层中的行星间隙:Alma的可观察性
机译:填补空白:启发(a)过渡原行星盘的清除机制,以及(b)本科理科学生的定量文盲率。
机译:现实冰地幔的X射线加工可以解释原文象磁盘中的气体丰富
机译:多环芳烃离子化作为气体的示踪剂流过原行星盘间隙