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Final List of 135 Registered Persons
Suggested session and affiliation summary
Session priority 25 Molecular Clouds 22 Massive Stars 19 Cores 18 Triggered SF 12 Chemistry 10 Envelopes 10 Filaments 10 Magnetic Fields 6 Disks	Affiliation 41 USA 38 Germany 11 France 9 Japan 9 UK 4 Canada 3 Austria 2 Netherlands 2 South Korea 2 Taiwan 2 Chile 2 Denmark 2 Mexico 2 Spain 1 Argentina 1 Brazil 1 Italy 1 Ireland 1 Netherlands 1 Russia

Waiting list

Chronologically ordered list of registered persons Some titles/contributions have been submitted to the SAC but are not given here.
#	Name/Affiliation	Suggested Contribution or Review	Suggested Sessions
135	H. Zinnecker NASA AMES/Univ. Stuttgart, USA/Germany	Do all massive stars form in clusters?	Massive Stars, Molecular Clouds, Cores, Triggered SF
134	A. Whitworth Cardiff Univ., UK	Mapping the Core Mass Function (CMF) into the Stellar IMF	Cores
133	M. Malygin MPIA Heidelberg, Germany	Frequency dependent opacity in the dust-free inner region of a circumstellar disk	Massive Stars
132	A. Goodman HSCA Cambridge, USA	Molecular Clouds Under Pressure	Molecular Clouds
131	F. Motte CEA/IRFU - CNRS/INSU - Univ. Paris Diderot	Linking the formation of molecular clouds and high-mass stars: the W43 case study	Molecular Clouds, Massive Stars, Filaments
130	H. Linz MPIA Heidelberg, Germany	The onset of star formation in IRDCs: From embedded Herschel point sources to early molecular outflows traced in SiO	Massive Stars Cores, Filaments
129	M. Hennemann AIM CEA Saclay, France	Cloud structure and (high-mass) star formation rate: HOBYS Herschel observations of massive ridges, their feeding subfilaments, and the evolution of massive dense cores	Massive Stars, Filaments, Envelopes, Cores
128	W. Fischer Univ. Toledo, USA	HOPS: Testing the Low-Mass Star Formation Paradigm in the Orion Molecular Clouds	Envelopes
127	A. Bacmann IPAG Grenoble, France		Chemistry
126	J. Kauffmann Jet Propulsion Laboratory, Pasadena, CA, USA	The Density Structure of Clouds: Large Samples, Star Formation Thresholds, and Theoretical Models	Molecular Clouds, Cores, Filaments
125	T. Haugboelle Univ. Copenhagen, Denmark	Large scale modeling of the ISM and the origin of stellar masses	Envelopes, Filaments, Molecular Clouds, Magnetic Fields
124	J. Kainulainen MPIA Heidelberg, Germany	Column density probability distributions as probes of atomic and molecular gas in the star-forming ISM	Molecular Clouds
123	T. Vasyunina Univ. Virginia, USA	Chemical composition and chemical processes in IRDCs	Chemistry, Massive Stars
122	R. Chen MPIfR Bonn, Germany	Formation of Molecular Clouds under Tidal Influence - the Case of Magellanic Bridge	Molecular Clouds, Massive Stars
121	A. Maury ESO Garching, Germany	First results from CaLYPSO: the IRAM Plateau de Bure Large Program on Class 0 protostars. A dive into the small-scale physics and chemistry of young envelopes, disks and outflows.	Envelopes, Disks, Chemistry
120	T. Troland Univ. Kentucky, USA	The Role of Magnetic Fields in Galactic GMCs	Magnetic Fields, Molecular Clouds
119	C. Battersby CASA, Univ. Colorado, USA	The Kinematics of Filaments and Their Role in High-Mass Star Formation	Filaments, Massive Stars, Molecular Clouds, Triggered SF
118	A. Hughes MPIA Heidelberg, Germany	Giant Molecular Clouds and Star Formation in M51	Molecular Clouds
117	J. Forbrich Vienna Univ./SAO, Austria/USA	Star formation rates from Galactic molecular clouds to galaxies	Molecular Clouds
116	C. Contreras CAR, Univ. Hertfordshire, UK	Extreme Variables in Star Forming Regions	Disks
115	P. Padoan ICREA&ICC, Barcelona, Spain	The Star Formation Rate of Molecular Clouds	Molecular Clouds, Filaments, Magnetic Fields, Cores
114	A. Schmiedeke Univ. Köln, Germany	Confronting theory with observation: The case of NGC6334I	Chemistry, Massive Stars
113	M. Kama AIAP Amsterdam, The Netherlands	The strange complexity of the protostar OMC-2 FIR 4 as revealed by Herschel/HIFI	Envelopes, Cores, Chemistry
112	M. Zamora-Aviles CRyA-UNAM Morelia, Mexico	An Evolutionary Model for the Star Formation Efficiency in Gravitationally Collapsing Molecular Clouds	Molecular Clouds, Envelopes, Triggered SF
111	A. Bracco IAS Orsay, France	Observing the magnetic field structure in the ISM with Planck	Magnetic Fields
110	E. Servajean Univ. Chile, Santiago, Chile	Characteristics of two very young massive star forming regions	Cores, Massive Stars
109	J. Pineda ESO/UK ARC Node, Univ. Manchester, UK	The Barnard 5 Star-forming Core: Embedded Filaments Revealed	Filaments, Cores, Chemistry, Envelopes
108	K. Iwasaki Nagoya University, Nagoya, Japan	Gravitational Fragmentation of Expanding Shells	Triggered SF
107	S. Glover ITA/ZAH Heidelberg, Germany	Is molecular gas necessary for star formation?	Molecular Clouds, Chemistry
106	S. Ragan MPIA, Heidelberg, Germany	From clouds to cores: kinematics in infrared-dark clouds	Molecular Clouds, Massive Stars, Cores
105	P. Clark ITA/ZAH Heidelberg, Germany	The origin of the characteristic mass for star formation	Cores, Filaments, Molecular Clouds
104	G. Parmentier MPIfR Bonn, Germany	The Massive Star Formation Limit in the Mass-Size Space of Molecular Structures	Massive Stars, Cores
103	C. Rodrigues INPE Sao Jose dos Campos, Brazil	Interstellar magnetic field around giant protostellar jets	Magnetic Fields
102	R. Shetty ITA Heidelberg Univ., Germany	Understading the X factor with MHD and radiative transfer simulations	Molecular Clouds, Cores, Chemistry
101	N. Hirano ASIAA Taipei, Taiwan	Two extremely young protostars in Barnard 1	Cores, Chemistry
100	D. Shibata Univ. Tokyo, Japan	Extracting the Effect of Low-Mass Star Formation on Deuterium Fractionation	Chemistry, Envelopes, Cores
99	M. Reiter Univ. Arizona Tucson, USA	Studying Intermediate Mass Star Formation in the Carina Nebula with HH Jets	Envelopes, Massive Stars, Triggered SF
98	B. Kelly Univ California, Santa Barbara, USA	What is the relation between the dust properties and temperature in molecular clouds?	Cores, Molecular Clouds, Chemistry
97	N. Smith Univ. Arizona/Steward Obs., USA	Feedback-driven star formation in the Carina Nebula	Triggered SF, Massive Stars,
96	M. Lundquist Univ. Wyoming, USA	A Galactic Sample of Intermediate-Mass Star-Forming Regions: Bridging the High- and Low-mass Regimes	Massive Stars
95	M. Gritschneder Univ. California Santa Cruz, USA	Feedback and Triggered Star Formation - From the Pillars of Creation to the Formation of the Solar System	Triggered SF, Filaments, Molecular Clouds
94	J-H. Shinn KASI Daejeon, South Korea	[Fe II] 1.64 um imaging observations of Jets and Outflows from Young Stellar Objects in the Carina Nebula	Triggered SF, Massive Stars
93	E. Vazquez-Semadeni CRA/UNAM Morelia, Mexico	Is the observed Galactic star formation rate compatible with gravitationally collapsing molecular clouds?	Molecular Clouds, Filaments
92	H-b. Li MPIA Heidelberg,Germany	The Link between Magnetic Fields, Filamentary Clouds and Star Formation Efficiency	Filaments, Magnetic Fields, Molecular Clouds
91	H. Kirk HSCfA Cambridge, USA	Filamentary Flows in the Serpens South Protocluster	Filaments, Massive Stars, Cores
90	L. Looney Univ. Illinois, USA	Changing the Paradigm for the Inner Envelope of Class 0 Protostars	Filaments, Envelopes, Cores
89	S. Pfalzner MPIfR Bonn, Germany	Formation of leaky clusters and OB associations	Massive Stars
88	Ra. Klein SOFIA-USRA Moffett Field, USA	Early Phases of Massive Star Formation in GLIMPSE and MIPSGAL	Massive Stars
87	E. Lee CITA Toronto, Canada	The Role of Large Scale Gravity and Turbulence in Star Formation	Molecular Clouds, Triggered SF
86	W. Schmidt IfA Göttingen, Germany	Support against gravity in magnetoturbulent gas	Molecular Clouds, Cores, Magnetic Fields
85	M. Alexander Univ Wyoming, USA	Is there an energy threshold for triggered star formation?	Triggered SF, Filaments
84	A. Kritsuk UC San Diego, USA	Understanding the Formation and Structure of Molecular Clouds	Molecular Clouds, Filaments, Magnetic Fields, Cores
83	A. Stutz MPIA Heidelberg, Germany	A new population of protostars discovered by Herschel	Envelopes, Cores
82	C. Beaumont Univ. Hawaii/Harvard, USA	Identifying Molecular Cloud Structures in Projected Data: What is Real, and What Isn't?	Molecular Clouds, Filaments
81	A. Coutens IRAP Toulouse, France	Deuterated water in low-mass protostars	Envelopes, Chemistry
80	J. Steinacker IPAG Grenoble/MPIA, France/Germany	Validity of the Bonnor-Ebert Approximation for B68: A core in 3D based on Herschel data	Cores
79	S-P. Lai NTH Univ., Taiwan	Discovery of Toroidal Magnetic Fields around Protostars in NGC1333 IRAS 4A from Dust Polarization Measurements	Magnetic Fields, Cores, Envelopes, Molecular Clouds
78	C-Y. Chen Univ. Maryland, USA	Ambipolar Diffusion and Prestellar Core Formation	Cores, Magnetic Fields, Filaments
77	M. Andersen IPAG Grenoble, France	A star cluster in its early stages	Massive Stars, Cores
76	K. Johnston MPIA Heidelberg, Germany	The interplay between molecular and ionized gas surrounding the massive embedded star AFGL 2591	Massive Stars, Disks, Triggered SF
75	T. Robitaille MPIA Heidelberg, Germany	A new grid of model spectral energy distributions for young stellar objects	Envelopes, Disks, Massive Stars
74	T. Downes Dublin City Univ., Ireland	Multifluid magnetohydrodynamic turbulence in molecular clouds	Molecular Clouds, Magnetic Fields
73	R. Smith ZAH/ITA Heidelberg, Germany	Collapsing Cores in Filaments and Massive Star Forming Regions	Cores, Filaments, Massive Stars
72	R. Aluzas Univ. Leeds, UK	Numerical simulations of multiple clouds interacting with a shock	Triggered SF
71	E. Vorobyov University of Vienna, Austria	Implications of the protostellar disk fragmentation	Disks
70	N. Kudryavtseva MPIA Heidelberg, Germany	Instantaneous starburst of the massive clusters Westerlund 1 and NGC 3603 YC	Massive Stars
69	J. Dutta ITA/ZAH Heidelberg, Germany	Angular Momentum Transport in Primordial Star Formation	Disks, Cores, Molecular Clouds, Envelopes
68	R. Crutcher Univ. Illinois, USA	CARMA Studies of Magnetic Fields in Dense Molecular Clouds	Magnetic Fields, Molecular Clouds
67	M. Walmsley INAF Firenze, Italy	Interpreting the "infall profile"	Cores, Chemistry
66	B. Commercon LERMA-ENS Paris, France	Collapse of Massive Magnetized Dense Cores using Radiation Magnetohydrodynmaics: Early Fragmentation Inhibition	Magnetic Fields, Massive Stars
65	R. Galvan-Madrid ESO Garching, Germany	The Structure of Accretion Flows in the Formation of Very Massive Stars	Massive Stars, Cores
64	T. Hill AIM Paris-Saclay, France	Filaments, ridges and a mini-starburst - HOBYS' view of high mass star formation with Herschel	Cores, Massive Stars, Molecular Clouds
63	J. Tige LAM Marseille, France	Starformation in NGC 6334 with Herschel datas	Massive Stars, Triggered SF
62	F. Renaud CEA/AIM Saclay, France	Star formation and feedback: a subparsec-resolution simulation of the Milky-Way	Triggered SF, Molecular Clouds, Cores
61	J. Ascenso ESO Garching, Germany	Star formation in giant complexes: The Cat's Paw Nebula	Triggered SF, Cores, Massive Stars
60	K. Tomisaka NAO Tokyo, Japan	Expected Observations of Star Formation Process: from Molecular Cloud Core to First Hydrostatic Core	Magnetic Fields, Cores
59	A. Ginsburg Univ. Colorado, USA	Surveying Pre-Stellar Gas in the Galactic Plane with Bolocam and Herschel	Cores, Filaments, Massive Stars, Molecular Clouds, Triggered SF
58	M.V. del Valle IAR La Plata, Argentina	The origin of the non-thermal emission in the jets of the massive protostar HH 80-81	Magnetic Fields, Massive Stars
57	E. Keto HSCfA, USA	Simplified oxygen-carbon chemistry in cold starless cores	Chemistry, Cores, Molecular Clouds
56	R. Kuiper JPL Pasadena, USA	Feedback in Massive Star Formation - On the effects of radiation pressure, stellar winds, and ionization on disk accretion, outflow launching, mass loss, and the upper mass limit of stars	Massive Stars, Triggered SF, Cores, Disks, Envelopes
55	A. Hacar OAN Madrid, Spain	Formation of dense cores in Taurus by fragmentation of velocity-coherent filaments	Filaments, Cores, Molecular Clouds
54	D. Seifried Hamburger Sternw., Germany	Disk formation in turbulent cores: Circumventing the magnetic braking catastrophe	Disks, Magnetic Fields, Massive Stars
53	K. Furuya Kobe Univ., Japan	Molecular Evolutions in the First Hydrostatic Core Stage Adapting Three-Dimensional Radiation Hydrodynamics Simulations	Chemistry, Cores, Envelopes
52	H.-F. Chiang Univ. Hawaii, USA	Interferometric Observations and Modeling of the Envelope around Class 0 Protostars	Envelopes, Cores, Disks
51	N. Sakai Univ. Tokyo, Japan	Chemical Diversity and its Evolution from Class 0 to Class I	Chemistry, Envelopes, Disks, Cores
50	F. Nakamura NAOJ, Japan	A Burst of Molecular Outflows From the Serpens South Protocluster	Triggered SF
49	Ri. Klein UC Berkeley/LLNL, USA	The Coupled Effects of Protostellar Outflows and Radiation Feedback on the Formation of Massive Stars	Massive stars, Triggered SF
48	Y. Aikawa Kobe University, Japan	From prestellar core to protostellar core: time dependence, deuterium fractionation, and disk formation	Chemistry, Envelopes, Disks
47	W-h. Hsu Univ. Michigan, USA	Missing Massive Stars: Statistically-significant Density Dependence of the IMF	Massive Stars, Filaments
46	M. Heyer Univ. Massachusetts, USA	The Velocity Structure of Molecular Clouds	Molecular Clouds, Filaments, Cores
45	Z. Nagy KAI & SRON, Netherlands	Extended warm and dense gas towards W49A: starburst conditions in our Galaxy?	Triggered SF, Massive Stars
44	M. Dunham Yale Univ., USA	Protostellar Luminosities and Accretion	Cores, Envelopes
43	C. McKee UC Berkeley, USA	The Protostellar Luminosity Function: Theory and Simulation	Cores, Envelopes
42	R. Mauersberger Joint ALMA Obs., Chile	ALMA Commissioning and Science Verification and Early Science	-
41	K. Tomida TGUAS/NAO, Japan	Radiation Magnetohydrodynamic Simulations of Protostellar Core Formation	Cores, Magnetic Fields, Disks
40	J. Tackenberg MPIA, Heidelberg, Germany	Starless clumps and the influence of near-by high-mass star formation	Triggered SF, Cores
39	T. Henning MPIA Heidelberg, Germany		-
38	K. Getman Pennsylvania State Univ., USA	The Chandra View of Triggered Star Formation in Bright Rimmed Clouds	Triggered SF
37	A. Pon Univ. Victoria, Canada	Molecular Tracers of Turbulent Shocks in Molecular Clouds	Molecular Clouds, Triggered SF, Chemistry
36	P. Myers HSCfA Cambridge, USA	Ages and birthrates of young clusters	Triggered SF, Cores, Massive Stars
35	K. Tassis MPIfR Bonn, Germany	Molecular Chemistry as a Probe of Pre-Stellar Core Dynamics: An Unprecedented Exploration of Models	Chemistry, Cores, Magnetic Fields
34	J. Carroll-Nellenback Univ. Rochester, USA	Comparing different molecular cloud formation mechanisms and subsequent evolution	Molecular Clouds
33	C.W. Lee Korea ASSI, South Korea	Internal motions in starless dense cores	Filaments, Molecular Clouds, Cores
32	G.-X. Li MPIfR Bonn, Germany	Molecular Outflow as an Entrainment Phenomenon	Massive Stars, Envelopes, Molecular Clouds
31	Y. Pavlyuchenkov RAS Moscow, Russia	Stochastic grain heating and mid-infrared emission in protostellar cores	Cores, Molecular Clouds, Envelopes
30	D. Kruijssen MPA Garching, Germany	The fraction of star formation occurring in bound stellar clusters	Triggered SF, Molecular Clouds, Massive Stars, Filaments
29	T. Gerner MPIA, Germany	Mapping the chemistry of the interstellar medium	Chemistry, Molecular Clouds, Cores
28	C. Dobbs Univ. Exeter, UK	Unbound molecular clouds and their evolution	Molecular Clouds
27	A. Lazarian Univ. Wisconsin, USA	Reconnection Diffusion: Fast Removal of Magnetic Field during Star Formation	Magnetic Fields, Molecular Clouds, Envelopes, Disks
26	G. Dopcke Univ. Heidelberg, Germany	Fragmentation of star-forming clouds at very low metallicities	Cores, Chemistry, Filaments, Disks
25	P. Hofner New Mexico Tech, USA	Jets from Massive Protostars	Massive Stars
24	S. Bihr MPIA, Germany	Temperature, kinematics and turbulence of infrared dark clouds (IRDCs) at high spatial resolution	Massive Stars, Cores, Molecular Clouds, Envelopes
23	S. Dib Imperial College, UK	Feedback Regulated Star Formation	Triggered SF, Massive Stars
22	S. Oey Univ. of Michigan, USA	The Salpeter Slope of the IMF Explained	Filaments, Massive Stars, Cores
21	E. Ntormousi Univ. Obs. Munich, Germany	Formation of filaments from colliding supershells	Filaments, Triggered SF, Molecular Clouds
20	D. Gouliermis ZAH/ITA, Germany	The hierarchical nature of star formation	Massive Stars, Triggered SF, Filaments, Molecular Clouds
19	E. van Dishoeck Leiden Observatory/MPE, The Netherlands	Water: from cores to disks	Chemistry, Envelopes
18	A. Wootten NRAO, USA	Time-Resolved AU-Scale Outflow Trajectories Traced by Masers in the IRAS16293-2422 Core	Cores, Disks
17	E. Bressert ESO/Univ. Exeter, Germany/UK	What the Spatial Distribution of Massive Stars tells us about Star Formation and the IMF	Massive Stars, Filaments
16	Z.-Y. Li Univ. Virginia, USA	Why is it difficult to form rotationally supported disks during the protostellar collapse of magnetized dense cores?	Disks, Magnetic Fields
15	S. Longmore ESO, Germany	HOPS + MALT90 + Hi-GAL: Probing star formation on a Galactic scale through mm molecular line and far-IR continuum Galactic plane surveys	Molecular Clouds
14	A. Burkert LMU, Uni. Obs., Germany	Self-regulated star formation in galaxies and the evolution of the molecular web	Molecular Clouds
13	A. Nordlund Niels Bohr Inst., Denmark	Star Formation and Chemical Yields in Giant Molecular Clouds	Triggered SF, Molecular Clouds, Filaments, Magnetic Fields
12	T. Haworth Univ. Exeter, UK	Radiation hydrodynamics of triggered star formation: the effect of the diffuse field	Triggered SF
11	M. Bate Univ. Exeter, UK	Short Review: Molecular Cloud Cores - Life and Collapse: Theory	Cores
10	J. Alves Viena Univ., Austria	Short Review: Molecular Cloud Cores - Life and Collapse: Observations	Cores
9	P. Goldsmith Jet Propulsion Lab., USA	Review: Molecular Clouds: Overview of their Structure and Evolution	Molecular Clouds
8	R. Banerjee Univ. Hamburg, Germany	Review: The Early Phases of Disc Formation and Disc Evolution	Disks
7	M. Krumholz Univ. California, USA	Review: Star Formation Feedback: The Good, the Bad, and the Confusing	Triggered SF
6	S. Yamamoto Univ. Tokyo, Japan	Review: Chemical diagnostics of the early phase of star formation	Chemistry
5	F. Heitsch Univ. North Carolina, USA	Review: The Role of Filaments for Core Formation	Filaments
4	R. Pudritz McMaster Univ., Canada	Review: Magnetic fields and the early stages of star formation	Magnetic Fields
3	H. Beuther MPIfAstronomie, Germany	Review: High-Mass Star Formation	Massive Stars
2	D. Johnstone NRCC, HIoAstrophysics, Canada	Review: Protostellar Envelopes	Envelopes
1	H. Yorke Jet Propulsion Lab., USA	Conference Summary	-