| No. |
Name |
Affiliation |
Contribution |
| P2 |
I. Baraffe |
Ecole Normale Superieure, Lyon, France, and University of Exeter, UK |
Very early stages of evolution of low mass stars and brown dwarfs: Effect of episodic accretion
|
| P3 |
A.O. Benz |
Institute of Astronomy, ETH Zurich, Switzerland
|
Results of Herschel Hydride Observations
|
| P4 |
A. Bik |
MPIA Heidelberg, Germany |
A spectroscopic census of the stellar content of high-mass star-forming regions
|
| P5 |
A. Burkert |
University Observatory Munich, Germany |
The ultimate fate of B68 and the origin and evolution of globules in the
Pipe nebula
|
| P6 |
P.C. Clark |
ITA, ZAH, Universität Heidelberg, Germany
|
The formation of prestellar cores
|
| P7 |
B. Commercon |
MPIA Heidelberg, Germany
|
Protostellar collapse: magnetic and radiative feedbacks on small scales collapse and fragmentation
|
| P8 |
E.D. Feigelson |
Pennsylvania State University, USA |
X-ray insights into the formation of stellar clusters
|
| P9 |
A. Hacar |
Observatorio Astronomico Nacional, Spain
|
Formation of Dense Cores in the Taurus Molecular Cloud
|
| P10 |
M. Hennemann |
CEA Saclay, France
|
Intermediate- to high-mass star formation in the Rosette Molecular Cloud and in Isolation as observed by Herschel and the PdBI
|
| P11 |
Th. Henning |
MPIA Heidelberg, Germany
|
The Earliest Stages of Massive Stars
|
| P12 |
J. Kainulainen |
Max-Planck-Institut für Astronomie, Germany
|
Probing the evolution of molecular cloud structure using dust column density data
|
| P13 |
H. Kirk |
Harvard - Smithsonian Center for Astrophysics, USA
|
Mass Segregation in Young Stellar Groups
|
| P14 |
P. Klaassen |
ESO Garching, Germany
|
Outflows from Massive Star Forming Regions
|
| P15 |
K.M. Kratter |
University of Toronto, Canada
|
Disks and the formation of stellar systems
|
| P16 |
L.E. Kristensen |
Leiden Observatory, The Netherlands
|
Water in low-mass star-forming regions - first Herschel results
|
| P17 |
R. Kuiper |
Max-Planck-Institut für Astronomie, Germany
|
Overcoming the radiation pressure barrier in the formation of massive stars via disk accretion
|
| P18 |
H. Linz |
MPIA Heidelberg, Germany |
Deeply embedded populations and thermal emission from IRDCs - the
Herschel view
|
| P19 |
A. Maury |
ESO Garching, Germany
|
PdBI subarcsecond observations of Class 0 protostars
|
| P20 |
M. Nielbock |
MPIA Heidelberg, Germany |
Photometric Calibration and Accuracy of the Herschel/PACS Photometer Camera
|
| P21 |
A. Nordlund |
NBI, Denmark |
Understanding the Star Formation Rate
|
| P22 |
N. Peretto |
Service d'Astrophysique CEA Saclay, Saclay, France |
Mapping dust properties across IRDCs with Herschel
|
| P23 |
R.E. Pudritz |
Origins Institute, McMaster University, Canada
|
The Early History of Disks, Outflows, and Binary Stars
|
| P23A |
S. Ragan |
Max-Planck-Institut für Astronomie, Heidelberg, Germany
|
High-Resolution Mapping the Kinematic and Temperature Structure in IRDCs
|
| P24 |
M. Reiter |
Steward Observatory, University of Arizona, Tucson, USA
|
Probing the Chemical and Kinematical Structure of High-mass Star-forming Cores
|
| P25 |
P. Schilke |
Universität zu Köln, Germany
|
From Cloud to Star Formation: the case of W43
|
| P26 |
R. Smith |
Institut für Theoretische Astrophysik Heidelberg, Germany
|
The Missing Link - Connecting Massive Stars to their Progenitor Cores
|
| P27 |
L. Testi |
ESO Garching/INAF-Arcetri, Germany/Italy
|
The early phases of star cluster formation
|
| P28 |
K. Tomida |
National Astronomical Observatory of Japan
|
Nested-Grid RMHD Simulation of Proto-stellar Collapse
|
| P29 |
T.A. van Kempen |
Harvard-Smithsonian, USA
|
The far-IR spectrum of low-mass protostars: Analysis of First results of the DIGIT and WISH Herschel Key programs
|
| P30 |
T. Vasyunina |
MPIA Heidelberg, Germany |
Molecular inventory of the Infrared Dark Clouds
|
| P31 |
C.M. Walmsley |
INAF, Osservatorio di Arcetri, Italy
|
CN, HCN, and HNC at high densities in prestellar cores
|
| P32 |
Y. Wang |
MPIA Heidelberg, Germany |
Different Evolutionary Stages of the Massive Star-Forming Region S255IR Complex
|
| P33 |
D. Wiebe |
Institute of Astronomy of the RAS, Moscow, Russia
|
Consistent Densities and Temperatures in Cores of Infrared Dark Clouds
|
| P34 |
E. Winston |
University of Exeter, Exeter, UK
|
Properties of YSOs in the NGC 1333 and Serpens Embedded Clusters
|
| P35 |
S. Yamamoto |
The University of Tokyo, Japan |
Line Survey of Low-Mass Star Forming Regions
|
