The
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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
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Program
Participants
Posters
Focus Groups
Big Questions
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EPoS 2014 Posters
P1
Christine Koepferl
The Star-formation Rate of the Central Molecular Zone determined from Young Stellar Objects
P2
Henrik Beuther
The carbon budget and formation signatures of molecular clouds
P3
Simon Bihr
W43 - How much neutral atomic hydrogen is hidden?
P4
Vivien Chen
Disk Accretion around the Massive Protostar IRAS 20126+4104
P5
Nichol Cunningham
What is Driving the Outflows in Massive Star Forming Regions?
P7
Emily Drabek-Maunder
Investigating outflow and cloud energetics in Ophiuchus and other GBS clouds
P8
Siyi Feng
Chemical substructure of high-mass star-forming regions
P9
Adam Ginsburg
Feeding a Massive Cluster along Filaments in W51
P10
Josep Girart
Magnetic Fields and Massive Star Formation
P11
Matthias Gritschneder
The Fate of Ionization Triggered Stars
P12
Jenny Hatchell
First JCMT Gould Belt Survey results on multiple systems
P13
Chat Hull
From clouds to cores to envelopes to disks: a multi-scale view of magnetized star formation
P14
Katharine Johnston
The structure and star-forming fate of the Galactic centre cloud G0.253+0.016
P15
Eric Keto
The formation of filaments by reconnection in magnetized sheets
P16
Alexei Kritsuk
Interstellar Turbulence, Molecular Clouds and Star Formation
P17
Diederik Kruijssen
An Uncertainty Principle for Star Formation - Putting direct constraints on the physics of cloud evolution, star formation and feedback
P18
Di Li
Physical and Chemical Properties of Massive Quiescent Cores in Orion
P19
Hendrik Linz
FIR lines from Herschel cores: state of the molecular and atomic gas
P20
Anna McLeod
Feedback of massive star formation: from simulations to observations
P21
Nickolas Moeckel
The formation of filamentary bundles in turbulent molecular clouds
P22
Markus Nielbock
Star Formation in the Norma Cloud
P23
Liubin Pan
The role of turbulence for dust growth in protostellar cores and disks
P24
Jaime Pineda
Turbulence dissipation and fragmentation in an isothermal filament: initial conditions for star formation
P25
Rene Plume
Results from the HEXOS Full Band Spectral Survey of Orion South
P26
Adele Plunkett
Outflows and clustered star formation on scales of cores to clouds
P27
Sarah Ragan
Core kinematics in infrared-dark clouds
P28
Thomas Robitaille
Characterizing the hierarchical structure of molecular clouds with dendrograms
P29
Thomas Stanke
Connecting Environment with Protostars with the Herschel Orion Protostar Survey
P30
Jeremy Tige
Massive Dense Cores in Molecular Clouds
P31
Kohji Tomisaka
Magnetohydrostatic Equilibrium Structure and Mass of Filamentary Isothermal Cloud Threaded by Lateral Magnetic Field
P32
Tatiana Vasyunina
Chemical variations in Infrared Dark Clouds: from starless cores to hot core candidates
P33
Ke Wang
Fragmentation at the Earliest Phase of Massive Star Formation
P34
Manuel Zamora-Aviles
Molecular Cloud evolution: Regulation of the Star Formation Rate by feedback from massive stars
The EPoS way: Large group, small room, remote location. Consider all aspects. Short talks, intense discussions.