NUMERICAL ASTROPHYSICS AND ITS ROLE IN STAR FORMATION
Cardiff, 19-23
January 2009
| NAME | INSTITUTE |
TALK/POSTER
TITLE |
| Alicia Aarnio |
Vanderbilt
University |
|
| Richard Allison |
Sheffield
University |
|
| Philippe André |
CEA/Saclay -
Service d'Astrophysique |
|
| Serena Emily Arena |
University
of Tuebingen |
SPH simulations of solid bodies
for studying planetesimal formation [P] |
| Rhianne Attwood |
Cardiff
University |
The role of turbulence and thermodynamics on star formation in molecular cloud cores [T] |
| Edouard Audit |
Service
d'Astrophysique, CEA/Saclay |
Radiative transfer using the
Moment Method, and its application to radiative shocks [T] |
| Manuel
Abelardo Zamora Aviles |
Centro de
Radioastronomia y Astrofisica (UNAM) |
|
| Ben Ayliffe |
University
of Exeter |
|
| Robi Banerjee |
Institute
for Theoretical Astophysics (ITA) University of Heidelberg |
Contemporary Star
Formation with the FLASH code [T] |
| Matthew Bate |
University of Exeter | School summary [T] |
| Christopher Batty |
Cardiff
University |
|
| Alberic Joos de ter Beerst |
CRAL (Centre de Recherche Astrophysique de LYON) |
|
| Thomas Bisbas |
Cardiff
University |
SPH simulations of expanding HII regions [T] |
| Ian Bonnell |
University
of St Andrews |
Cluster
and distributed modes and the efficiency of star formation [T] |
| Sylvain Bontemps |
Observatoire
de Bordeaux |
|
| Chris Brunt |
Exeter University | |
| Andrew Burgess |
LAOG,
France |
|
| Ana Duarte Cabral |
Jodrell Bank Centre for
Astrophysics
University of Manchester
|
|
| Marilena Caramazza |
INAF
Osservatorio Astronomico di Palermo |
|
| Cátia Cardoso |
Exeter
University |
|
| Annabel
Cartwright |
Cardiff
University |
The
effect of Poisson noise on the accuracy of SPH calculations: does
increasing particle numbers help? [T] |
| Paola Caselli |
School of Physics &
Astronomy
University of Leeds
|
Pedagogical
Talk on Diagnostic Chemistry [T] |
| Seung-Hoon Cha |
Theoretical
Astrophysics Group, Dept. of Physics and Astronomy, University of
Leicester |
Kelvin-Helmholtz
instability with Godunov-type SPH [P] |
| Gilles Chabrier |
ENS-Lyon,
France |
The basics of the early
evolution of young objects: from the proto-star/BD to the PMS phase [T] |
| Yilen Gomez
Maqueo Chew |
Vanderbilt
University |
|
| María Dolores Mata
Chávez |
Centro de
Radioastronomía y Astrofísica (UNAM) |
|
| Paul C. Clark | ITA Universitaet Heidelberg | The formation of discs in clusters [T] |
| Benoît Commerçon |
CEA Saclay
(France) |
Protostellar
collapse: numerical methods comparison and development [T] |
| Peter Cossins |
University
of Leicester |
|
| Timea Csengeri |
CEA-Saclay |
Origin
of high-mass stars and clusters in DR21(OH) [P] |
| James Dale |
Astronomical Institute
Czech Academy of Sciences
|
Stellar
feedback - modelling HII
regions, stellar winds and fragmenting shells in
SPH [T] |
| Clare Dobbs |
University
of Exeter |
How Do You Solve a Problem Like Molecular Cloud Formation? [P] |
| Kevin Douglas |
University
of Exeter |
How Do You Solve a Problem Like Molecular Cloud Formation? [P] |
| Davide Elia |
Observatório
Astronómico de Lisboa Centro de Astronomia e Astrofísica da Universidade de Lisboa, Portugal |
|
| Barbara Ercolano |
Institute of Astronomy
University of Cambridge
|
Geometry
Independent Radiative Transfer through Gas and Dust using the Monte
Carlo method [T] |
| Christoph Federrath |
ITA/ZAH
Heidelberg |
Interstellar
Turbulence: Solenoidal
versus Compressive Forcing [P] |
| Pau Frau-Mendez |
Institut de
Ciencies de l'Espai (ICE/CSIC), Spain |
|
| Duncan Forgan |
Institute for Astronomy
University of Edinburgh, SUPA
|
Introducing
a Hybrid Method of Radiative Transfer for SPH [T] |
| Sebastien Fromang |
CEA
Saclay, France |
Numerical
dissipation in MHD turbulence
simulations performed with ZEUS [T] |
| Evghenii Gaburov |
Leiden
Observatory |
A star cluster on a desktop (1) [T] |
| Simon Glover |
Institut fuer Theoretische
Astrophysik University of Heidelberg |
Simulating
chemically reactive flows in astrophysics [T] GPM Lagrangian Hydrodynamics [P] |
| Joana Filipa Inês Gomes |
Centro de
Astronomia e Astrofísica da Universidade de Lisboa (CAAUL) |
|
| Manuel Neri Gómez |
Centro de Radioastronomía
y Astrofísica
UNAM
|
Physical properties of interstellar atomic dense structures from turbulent simulations [P] |
| Simon Goodwin |
Sheffield
University |
The
collapse of cold fractal star clusters [T] |
| Jane Greaves |
|
|
| Oliver Gressel |
Queen Mary
University London |
Magnetic
field amplification in turbulent flows [T] |
| Matthias Gritschneder |
University
Observatory, Munich |
Ionization in SPH Simulations: iVINE and
VINERY [T] |
| Tim Harries |
University
of Exeter |
The
simulation of line emission from protostars and discs [T] |
| Calen Barnett Henderson |
Vanderbilt
University
|
A
Search for Pre-Main Sequence Eclipsing Binary Stars in the Lagoon
Nebula [P] |
| Patrick Hennebelle |
Ecole normale superieure
Observatoire de Paris
|
Pedagogical talk on Finite
Difference
Hydrodynamics [T] |
| Alexander Hobbs |
Theoretical
Astrophysics Group University of Leicester |
|
| Seyit Hocuk |
Kapteyn Astronomical Institute
University of Groningen
|
The Metallicity and Rotational
Moment
Dependence of Molecular
Cloud Fragmentation [P] |
| Ella Hopewell |
INAF-Osservatorio
Astronomico di Palermo |
|
| David Hubber |
Oslo
University/Sheffield University |
"SPH in 60 mins". Pedagogical
talk on SPH [T] |
| Kazunari Iwasaki |
Osaka
University |
|
| Richard Jackson |
Astrophysics
Group, Keele University UK |
Are
the spin axes of stars randomly aligned in young clusters? [P] |
| Anne-Katharina
Jappsen |
Cardiff
University |
Influence of thermal properties on star formation [T] |
| Rob Jeffries |
Keele
University |
Tests
of Early Stellar Evolution Models [T] |
| Amit Kashi |
Physics Department
Technion – Israel Institute of
Technology
|
Physical
processes during the periastron passage of Eta Carinae [P] |
| Jongsoo Kim |
Canvendish Astrophysics Group
&
Korea Astronomy and Space
Institute
|
An Explicit Scheme for Incorporating Ambipolar
Diffusion in a Magnetohydrodynamics Code [P] |
| Jason Kirk |
Cardiff
University |
|
| Pamela Klaassen |
ESO |
Rotation in Regions of Massive Star
Formation [P] |
| Vera Konyves |
CEA/Saclay,
SAp |
|
| Thijs Kouwenhoven |
University
of Sheffield |
A
star cluster on a desktop (2) [T] |
| M.Abdul Latif |
Kapteyn
Astronomical Institute |
|
| Giuseppe Lodato |
University of Leicester (UK)/
University of Milan (Italy)
|
Angular momentum transport in
protostellar discs: clues from SPH simulations of self-gravitating
discs [T] |
| Ana Lopez-Sepulcre | INAF - Osservatorio Astrofisico di Arcetri | |
| Quang Nguyen Luong |
Service de
astrophysique, Saclay, France |
|
| Andres Suarez
Madrigal |
Centro de
Radioastronomia y Astrofisica UNAM |
Wavelet
analysis of a molecular
cloud
in numerical simulations [P] |
| George Mamatsashvili |
Institute
for Astronomy, University of Edinburgh |
Vortices in self-gravitating gaseous
discs [P] |
| Thomas Maschberger |
Institute of
Astronomy, Cambridge, UK |
|
| Mark McCaughrean |
University of Exeter | |
| Andrew McLeod |
Cardiff
University |
|
| Farzana
Meru |
University
of Exeter |
|
| Milica Milosavljevic |
Institute
for Theoretical Astrophysics, Heidelberg, Germany |
Stability of organic molecules
against shocks in the early Solar nebula [P] |
| Nickolas Moeckel |
University
of St Andrews |
Testing
binary formation scenarios with
SPH [T] |
| Takanori Nagakura |
National
Astronomical Observatory of Japan |
Evolution
of a supernova shell and triggered star formation in low-metallicity [P] |
| David Nutter |
Cardiff
University |
JCMT Gould Belt Legacy Survey [P] |
| Catarina
Alves de Oliveira |
LAOG
(Laboratoire d'Astrophysique de Grenoble) |
|
| James Owen |
IOA,
Cambridge |
|
| Jan Palous |
Astronomical
Institute, Academy of Sciences of the Czech Republic |
Expanding shells, massive star
clusters and gas stripping of galaxies [T]
|
| Richard Parker |
Sheffield
University |
The
Initial Binary Population in Star Clusters [T] |
| Stephanie Pekruhl |
University
Observatory, LMU Munich |
|
| Dieter Poelman |
University
of St. Andrews |
Rotational
line emission from water in protoplanetary disks [T] |
| Krisada Rawiraswattana |
Sheffield University | |
| Basmah Riaz |
Instituto de
Astrofisica de Canarias |
A study of a
depply-embedded low-mass protostellar system in the B59 molecular cloud
[P] |
| Ken Rice |
Institute for Astronomy
University of Edinburgh
|
Using SPH, with realistic thermodynamics, for
simulations of star and planet formation [T] |
| Boyke Rochau |
Max Planck
Institute for Astronomy Heidelberg, Germany |
Starburst
Cluster of the Milky Way [P] |
| Anooshiravan Roozrokh |
Sharif
University of Technology Iran |
|
| David Rundle |
University
of Exeter |
|
| Giuseppe Germano Sacco |
INAF-Osservatorio
Astronomico di Palermo |
Hydrodynamic
modeling of accretion shock on CTTSs [P] |
| Eugenio Schisano |
INAF
Osservatorio Astronomico di Capodimonte |
|
| Vojtech Sidorin |
Astronomical Institute of
the Academy of Sciences of the Czech Republic
|
Multiwavelength
study of
expanding H
I shells in the Milky Way [P] |
| Robert Simpson |
Cardiff
University |
|
| Rowan J Smith |
University
of St-Andrews |
Tracing the Evolution of Pre-Stellar Clumps
[P] |
| Loredana Spezzi |
Research and
Scientific Support Department, European Space Agency (ESTEC) |
Probing
the mass accretion process in the field of SN1987A [P] |
| Dimitris
Stamatellos |
Cardiff
University |
The formation of brown dwarfs in discs: physics and numerics [T] |
| Mario Tafalla |
Observatorio
Astronomico Nacional, Spain |
Determining
molecular abundances in
starless cores [T] |
| Stefanie Walch |
Cardiff
University |
The
formation and early
evolution of protostellar disks around low-mass stars [T] |
| Malcolm Walmsley |
Arcetri |
The
competition between depletion and
collapse [T] |
| Derek Ward-Thompson |
Cardiff
University |
|
| Carsten Weidner |
University
of St. Andrews |
|
| Lucy A. Wilcock |
Cardiff
University |
|
| Elaine Winston |
University
of Exeter |
|
| Ant
Whitworth |
Cardiff
University |
|
| Richard Wunsch | Cardiff University | Gravitational fragmentation of the expanding shell [T] |
| Bernd Völkl |
ITA
Heidelberg |
Radiative
Cooling with FLASH [P] |