EPoS2022 Posters

Each poster space has the dimension

750 mm width × 1250 mm height
29.5 inch × 49.2 inch

A0 is too large:
841 mm × 1189 mm
33.1 inch × 46.8 inch

A1 fits but leaves some space:
594 mm × 841 mm
23.4 inch × 33.1 inch

P01	Ahmad Ali	Star cluster formation and feedback in different galactic environments
P02	Maite Beltrán	Self-similarity of the magnetic field in G31.41+0.31 from core to circumstellar scales
P03	Asmita Bhandare	Mixing is easy: new insights on gas and dust dynamics during disc formation
P04	Gordian Edenhofer	Interstellar dust in 3D at parsec-scale resolution out to 1.25 kiloparsecs in distance
P05	Jan Forbrich	Almost like home: deep CO isotopologue, dust continuum and HCN observations of resolved Giant Molecular Clouds in the Andromeda Galaxy
P06	Brandt Gaches	The High-resolution Accretion Disks of Embedded Protostars (HADES) simulations: Accretion flows onto embedded protostars
P07	Josefa Elisabeth Großschedl	The evolution of velocity dispersion in OB associations - The case of Sco-Cen
P08	Rebecca J. Houghton	The star formation rate in the Galactic Centre using JWST imaging
P09	Katharine G. Johnston	Resolving the disk-jet accretion connection for forming massive stars
P10	Jens Kauffmann	Unraveling Molecular Cloud Populations and Lifecycles with LEGO and the Haystack Telescope
P11	Wonju Kim	CASCADE: Unveiling the photodissociation chemistry and feedback in DR18
P12	Alva Kinman	The Core Mass Function in the Galactic Center
P13	Rolf Kuiper	On the metallicity-dependence of radiation forces and photoionization feedback in massive star formation
P14	Shih-Ping Lai	Searching for young stellar objects through SEDs by machine learning
P15	Hua-bai Li	A Unified Explanation of Zeeman Measurements and Polarized Thermal Dust Emission
P16	Shanghuo Li	High-order multiplicity formation in high-mass stellar protocluster
P17	Hendrik Linz	Episodic accretion in high-mass star formation: Follow-up on accretion-burst sources
P18	Núria Miret-Roig	Synchronising stellar clocks. A new observable for probing star formation and dispersion
P19	Sanghyuk Moon	When and How Do Prestellar Cores Collapse? Critical Conditions and Collapse Dynamics from Analytic Modeling and Numerical Simulations
P20	Luca Moscadelli	The 3D velocity and magnetic fields of a MHD disk-wind around a forming star
P21	Alice Nucara	Probing Star-Formation Mechanisms in Massive Star-Forming Regions: Bridging Observations and Simulations through the Rosetta Stone Project
P22	Giovanni Sabatini	First ALMA Maps of Cosmic-Rays Ionization Rate in High-mass Star-forming Regions
P23	Jinshi Sai	Influence of Turbulence in Dense Cores on the Formation and Evolution of Protostellar Disks
P24	Alberto Sanna	Gas infall via accretion disk - late findings
P25	Kamber Schwarz	Evidence of Enhanced Ionization in Protostellar Envelopes
P26	Cameren Swiggum	Unveiling the majority origins of young stellar clusters in the local Milky Way and their role in shaping interstellar structure
P27	Travis J. Thieme	The Dynamics of Infall in Class 0 Protostars: A Case of Multiple Streamers in Lupus 3-MMS
P28	Benjamin Thomasson	Analytical model of hierarchical fragmentation within molecular clouds: towards a new perspective?
P29	Yao-Lun Yang	Chemical Evolution in Embedded Protostars: Ice Chemistry Unveiled by JWST
P30	Annie Zavagno	Machine learning for filament detection