The
E
arly
P
hase
o
f
S
tar Formation
The MPIA conference series at Ringberg Castle
2006
2008
2010
2012
2014
2016
2018
2020
2022
2024
2026
Objectives
Registered
Program
Participants
Posters
Focus Groups
Big Questions
Download
SAC/LOC
EPoS 2014 Download
Reviews
Hector Arce
Protostellar Outflows and their Effect on Star Formation, from Disk to Cloud Scales
Shantanu Basu
Magnetic Fields from Cloud Fragmentation to Disks
Edith Falgarone
Turbulence
Frederique Motte
From filamentary clouds to fibers feeding individual cores: how do filaments impact cloud and star formation?
Nicolas Peretto
The importance of cloud fragmentation and gas dynamics for the formation of massive stars
Mario Tafalla
Dense cores: from their internal structure to their connection with the surrounding cloud
Joao Alves
Conference Summary
Talks
Christian Fendt
Jet launching: MHD simulations of the accretion-ejection structure
Katharine Johnston
The structure and star-forming fate of the Galactic centre cloud G0.253+0.016
Rolf Kuiper
Quantifying the feedback effects of protostellar outflows and radiation pressure in massive star formation
Viviana Rosero
Deep Radio Continuum Observations of Massive Protostars: A Search for Jets
Sarah Sadavoy
Evidence of Feedback? Class 0 Protostellar Fraction and Environment in the Perseus Molecular Cloud
Kohji Tomisaka
Magnetohydrostatic Equilibrium Structure and Mass of Filamentary Isothermal Cloud Threaded by Lateral Magnetic Field
Posters
Adam Ginsburg
Feeding a Massive Cluster along Filaments in W51
Jennifer Hatchell
First JCMT Gould Belt Survey results on multiple systems
Chat Hull
From clouds to cores to envelopes to disks: a multi-scale view of magnetized star formation
Alexei Kritsuk
Interstellar Turbulence, Molecular Clouds and Star Formation
Di Li
Physical and Chemical Properties of Massive Quiescent Cores in Orion
Adele Plunkett
Outflows and clustered star formation on scales of cores to clouds
Ke Wang
Fragmentation at the Earliest Phase of Massive Star Formation
The EPoS way: Large group, small room, remote location. Consider all aspects. Short talks, intense discussions.