Man

Graeme Nicholas Candlish

Professor

UNIVERSIDAD DE VALPARAISO

Valparaíso, Chile

Líneas de Investigación


Cosmology; Gravitation; Galaxy formation/evolution

Educación

  •  BSc (Hons) Astrophysics, UNIVERSITY OF EDINBURGH. Reino Unido, 2002
  •  MSc (Distinction) Theoretical Physics, IMPERIAL COLLEGE OF SCIENCE, TECHNOLOGY & MEDICINE. Reino Unido, 2005
  •  Theoretical Physics, UNIVERSITY OF NOTTINGHAM. Reino Unido, 2010

Experiencia Académica

  •   Professor Full Time

    UNIVERSIDAD DE VALPARAISO

    2016 - At present

Experiencia Profesional

  •   Postdoctoral Researcher

    Universidad de Chile

    Chile

    2015 - 2016

  •   FONDECYT Fellow

    Universidad de Concepción

    Chile

    2012 - 2015

  •   Scientist

    UK Met Office

    Reino Unido

    2010 - 2012

  •   Profesor Full Time

    Universidad de Valparaíso

    Valparaíso, Chile

    2016 - At present


 

Article (16)

Discovery of ram-pressure stripped gas around an elliptical galaxy in Abell 2670
Phase-space analysis in the group and cluster environment=> time since infall and tidal mass loss
The Extended Baryonic Halo of NGC 3923
Could Segue 1 be a destroyed star cluster? - a dynamical perspective
MUSE-INGS on AM1354-250=> COLLISIONS, SHOCKS, and RINGS
The velocity field in MOND cosmology
Weighing the galactic disc using the Jeans equation=> lessons from simulations
BUDHIES II=> a phase-space view of HI gas stripping and star formation quenching in cluster galaxies
Simple and accurate modelling of the gravitational potential produced by thick and thin exponential discs
The difficult early stages of embedded star clusters and the importance of the pre-gas expulsion virial ratio
The sensitivity of harassment to orbit=> mass loss from early-type dwarfs in galaxy clusters
Life and death of a hero - lessons learned from modelling the dwarf spheroidal hercules=> An incorrect orbit?
Phase mixing due to the Galactic potential=> steps in the position and velocity distributions of popped star clusters
RAyMOND=> An N-body and hydrodynamics code for MOND
The influence of ram pressure on the evolution of tidal dwarf galaxies
Ursa Major II - reproducing the observed properties through tidal disruption

Proyecto (2)

Fortalecimiento de la física y la computación científicia en el Instituto de Física y Astronomía
USING SIMULATIONS TO UNDERSTAND GALAXY FORMATION AND EVOLUTION
1
Graeme Candlish

Professor

UNIVERSIDAD DE VALPARAISO

Valparaíso, Chile

1
Thomas Puzia

Associate Professor

Institute of Astrophysics

PONTIFICIA UNIVERSIDAD CATOLICA DE CHILE - DPTO. ASTRONOMIA Y ASTROFISICA

Santiago, Chile