Man

Diego Jose Munoz Anguita

Profesor Asistente

Universidad Adolfo Ibánez

Santiago, Chile

Líneas de Investigación


Theoretical Astrophysics; Accretion Disks; Planet Formation; Black Hole Binaries; Orbital Dynamics

Educación

  •  Astronomia, UNIVERSIDAD DE CHILE. Chile, 2004
  •  Astronomia, UNIVERSIDAD DE CHILE. Chile, 2006
  •  Astronomy, HARVARD UNIVERSITY. Estados Unidos, 2008
  •  Astronomy and Astrophysics, HARVARD UNIVERSITY. Estados Unidos, 2013

Experiencia Académica

  •   Research Associate Full Time

    CORNELL UNIVERSITY

    Ithaca, NY, Estados Unidos

    2013 - 2016

  •   Visiting Researcher Full Time

    TECHNION-ISRAEL INSTITUTE OF TECHNOLOGY

    Haifa, Israel

    2016 - 2017

  •   Visiting Researcher Full Time

    UNIVERSITY OF ARIZONA

    Tucson, AZ, Estados Unidos

    2017 - 2017

  •   CIERA Prize Fellow Full Time

    NORTHWESTERN UNIVERSITY

    Evanston, IL, Estados Unidos

    2017 - 2021

  •   Assistant Research Professor Part Time

    NORTHWESTERN UNIVERSITY

    Evanston, IL, Estados Unidos

    2021 - At present

  •   Assistant Professor Full Time

    UNIVERSIDAD ADOLFO IBANEZ

    Facultad de Ingeniería y Ciencias

    Santiago, Chile

    2021 - At present

Experiencia Profesional

  •   Asistente graduado de investigacion

    Harvard University

    Estados Unidos

    2006 - 2013

  •   Investigador Asociado Full Time

    Cornell University

    Ithaca, Estados Unidos

    2013 - 2016

  •   CIERA Fellow Full Time

    Northwestern University

    Evanston, Estados Unidos

    2017 - 2021

  •   Visiting Postdoctoral Researcher Full Time

    University of Arizona/Technion

    Tucson, AZ, Estados Unidos

    2016 - 2017

  •   Assistant Research Professor Part Time

    Northwestern University

    Evanston, IL, Estados Unidos

    2021 - At present

  •   Assistant Professor Full Time

    Universidad Adolfo Ibañez

    Santiago, Chile

    2021 - At present


 

Article (22)

A Disk-driven Resonance as the Origin of High Inclinations of Close-in Planets
Circumbinary Accretion from Finite and Infinite Disks
Inner Boundary Condition in Quasi-Lagrangian Simulations of Accretion Disks
Kozai Migration Naturally Explains the White Dwarf Planet WD1856 b
Long-lived Eccentric Modes in Circumbinary Disks
Hydrodynamics of Circumbinary Accretion: Angular Momentum Transfer and Binary Orbital Evolution
Statistical Trends in the Obliquity Distribution of Exoplanet Systems Diego
PLANETARY ENGULFMENT AS A TRIGGER FOR WHITE DWARF POLLUTION
Viscous hydrodynamics simulations of circumbinary accretion discs: variability, quasi-steady state and angular momentum transfer
Improving the convergence properties of the moving-mesh code AREPO
PULSED ACCRETION ONTO ECCENTRIC AND CIRCULAR BINARIES
The formation efficiency of close-in planets via Lidov-Kozai migration: analytic calculations
Stellar orbit evolution in close circumstellar disc encounters
Suppression of extreme orbital evolution in triple systems with short-range forces
Survival of planets around shrinking stellar binaries
ALMA OBSERVATIONS OF THE T TAURI BINARY SYSTEM AS 205: EVIDENCE FOR MOLECULAR WINDS AND/OR BINARY INTERACTIONS
Planet-disc interaction on a freely moving mesh
Multidimensional, compressible viscous flow on a moving Voronoi mesh
THE CIRCULAR POLARIZATION OF SAGITTARIUS A* AT SUBMILLIMETER WAVELENGTHS
CfA3: 185 TYPE Ia SUPERNOVA LIGHT CURVES FROM THE CfA
An X-ray, infrared, and submillimeter flare of Sagittarius A*
Massive clumps in the ngc 6334 star-forming region
22
Diego Munoz

Profesor Asistente

Universidad Adolfo Ibánez

Santiago, Chile

3
Cristóbal Petrovich

Assistant professor

Instituto de Astrofísica

Pontificia Universidad Católica de Chile

Santiago, Chile

1
Guido Garay

Profesor Titular

Astronomy

Universidad de Chile

Santiago, Chile

1
Diego Mardones

UNIVERSIDAD DE CHILE

Santiago, Chile