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Plan de Negocio para la Realización de Salón y Jardín de Eventos Sociales “Casa Bonita”

Authors
Publisher
Universidad de Chile
Publication Date
Keywords
  • Gestión Y Dirección De Empresas

Abstract

Observations of gas flows inside a protoplanetary gap Simon Casassus1, Gerrit van der Plas1, Sebastian Perez M.1, William R.F.Dent2,3, Ed Fomalont4, Janis Hagelberg5, Antonio Hales2,4, Andre´s Jorda´n6, Dimitri Mawet3, Francois Me´nard7,8, Al Wootten4, David Wilner9, A. Meredith Hughes 10, Matthias R. Schreiber11, Julien H. Girard3, Barbara Ercolano12 Hector Canovas11, Pablo E. Roma´n13, Vachail Salinas1 1. Departamento de Astronomı´a, Universidad de Chile, Casilla 36-D, Santiago, Chile 2. Joint ALMA Observatory, Alonso de Co´rdova 3107, Vitacura 763-0355, Santiago - Chile 3. European Southern Observatory (ESO), Casilla 19001, Vitacura, Santiago, Chile 4. National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903-2475, USA 5. Observatoire de Gene`ve, Universite´ de Gene`ve, 51 ch. des Maillettes, 1290, Versoix, Switzerland 6. Departamento de Astronomı´a y Astrofı´sica, Pontificia Universidad Cato´lica de Chile, Santiago, Chile 7. UMI-FCA, CNRS / INSU France (UMI 3386) , and Departamento de Astronomı´a, Universidad de Chile, Santiago, Chile. 8. CNRS / UJF Grenoble 1, UMR 5274, Institut de Plane´tologie et dAstrophysique de Grenoble (IPAG), France 9. Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 USA 10. Department of Astronomy, U. C. Berkeley, 601 Campbell Hall, Berkeley, CA 94720 11. Departamento de Fı´sica y Astronomı´a, Universidad Valparaiso, Av. Gran Bretana 111, Valparaiso, Chile. 12. University Observatory, Ludwig-Maximillians University, Munich. 1 ar X iv :1 30 5. 60 62 v1 [ as tro -p h.G A] 2 6 M ay 20 13 13. Center of Mathematical Modeling, University of Chile, Av. Blanco Encalada 2120 Piso 7, Santiago, Chile. Gaseous giant planet formation is thought to occur in the first few million years fol- lowing stellar birth. Models? predict that the process carves a deep gap in the dust component (shallower in the gas?, ?, ?). Infrared observations of the disk around

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