Posters
Poster information
- Presenters will have access to poster (vertical) walls of 1m (wide) x 2m (long)
- We encourage posters to be printed in A0 (vertical) format
- Special poster sessions will be dedicated for discussions
- The best two posters at the conference will be awarded with a poster prize and their PI will be invited to present their work in contributed talk by the end of the conference.
- There will be no poster presentation. Instead, there will be 2 dedicated poster sessions. Also, the posters will be accessible in every single coffee break.
Poster distribution in SR03 & SR05
Emergence of high-mass stars in complex fiber networks (EMERGE)
| ID | Author | Title |
|---|---|---|
| E1 | Hacar | EMERGE I. Early ALMA survey |
| E2 | Bonanomi | EMERGE II. The need of data combination |
| E3 | Socci | EMERGE III. Fiber networks in Orion |
| E4 | Socci | EMERGE IV. Environmental dependence of the fiber widths |
| E5 | Hacar | EMERGE V. From filaments to spheroids - the origin og HFS systems |
| E6 | Bonanomi | EMERGE VI. Turbulence dissipation and the origin of fibers |
Extragalactic star formation
| ID | Presenter | Title |
|---|---|---|
| X1 | Facchini | A census of seemingly isolated massive stars in nearby star forming galaxies |
| X2 | He | The Structure of Molecular Gas in PHANGS-ALMA Galaxies: Cloud Spacing, Two-Point Correlation, and Stacked Intensity Profiles |
| X3 | Jarvis | Star Formation, ISM Structure, and Ionizing Photon Escape in M33’s HII Regions |
| X4 | Marchuk | Different perspectives to specific star formation in and between spiral arms in galaxies |
| X5 | Neumann | Is Star Formation Universal? Lessons from Dense Gas in Nearby Galaxies with PHANGS-ALMOND |
| X6 | Wong | Resolved star formation scaling relations and gas-phase metallicity |
| X7 | Zakardjian | Estimating the dense gas mass of molecular clouds using spatially unresolved 3 mm line observations |
Galactic star formation
| ID | Presenter | Title |
|---|---|---|
| G1 | Benedettini | Kinematics in high-mass forming clumps: velocity field in ALMAGAL sources |
| G2 | Buddhacharya | What controls the star formation in Cloud E/F with ACES? |
| G3 | Fukaya | 1000 au-scale filamentary structures and cluster formation in Corona Australis revealed with ALMA |
| G4 | Großschedl | The Temporal Evolution of Velocity Dispersion Correlates with Periods of Heightened Star Formation Rate in Sco-Cen |
| G5 | Immer | Not Your Typical Disk: ALMA unveils an expanding, ring-shaped structure in G23.6-0.13 |
| G6 | Jones | Weighing protostellar cores with precision: uncovering the temperatures of high-mass star forming cores in ALMAGAL |
| G7 | Joó | Earliest stages of star formation in the brightest Planck compact sources |
| G8 | Karoly | The JCMT BISTRO Survey: Magnetic Fields Align with Orbital Structure in the Galactic Center |
| G9 | Kim | The internal and external impact of stellar feedback: from dense molecular clumps to OB-associated molecular clouds |
| G10 | Lee | Characterizing influence of outflow feedback in high-mass star-forming regions |
| G11 | Logue | ALMA EGO-10: Continuum Results from a 1.3 mm Imaging Survey of a Sample of Massive Protoclusters |
| G12 | Luo | The Formation of Low-Mass Multiple Protostellar Systems In the Milky Way |
| G13 | Marton | Discovering the hidden diversity of young stellar objects with unsupervised machine learning techniques |
| G14 | Mininni | How well molecules trace the continuum emission? A statistical study on the ALMAGAL sample |
| G15 | Rottensteiner | Investigating the kinematics and dynamical evolution of NGC 2024 with infrared proper motions |
| G16 | Sanhueza | The Magnetic Field at the Onset of High-mass Star Formation |
| G17 | Schilke | High-mass disks at high resolution with ALMA - toward a statistical sample |
| G18 | Sung | Environmental Impact on YSO Populations in a SED-Based Comparative Study |
| G19 | Traficante | Understanding Accretion Efficiency Across Scales in Massive Star Formation: First Results from the ALMAGAL Survey |
| G20 | Tsilia | Exploring Euclid capabilities to constrain the substellar IMF |
| G21 | Vázquez-Semadeni | The meaning of star formation efficiency in accreting clouds: gaseous and stellar mass evolution |
| G22 | Wallace | The ALMAGAL Hierarchical Structure Catalog: Investigating the multi-scale fragmentation of clumps throughout the Galaxy |
Interstellar medium
| ID | Presenter | Title |
|---|---|---|
| I1 | Alquicira Peláez | Numerical evolution of molecular outflow IRAS 04166+2706 |
| I2 | Asano | ALMA Multi-J CO observations of molecular clouds associated with the LMC SNR N63A |
| I3 | Huppenkothen | Modelling the neutral phases of the interstellar medium in galaxy simulations |
| I4 | Kaiser | Faraday rotation and magnetic field coherence: The impact of ISM properties |
| I5 | Keilmann | Reassessing the [CII]-Deficit in RCW79 |
| I6 | Piecka | Low density ISM flows within the Local Bubble and the Orion-Eridanus Superbubble |
| I7 | Sano | Discovery of Molecular Filaments Embedded within Supernova Remnants |
| I8 | Teh | From Expansion to Collapse: Exploring Stellar Feedback and Bubble Dynamics with TRINITY |
Molecular clouds
| ID | Presenter | Title |
|---|---|---|
| C1 | Abe | A Novel Mechanism to Drive Turbulence in Massive and Magnetized Star-forming Filaments. |
| C2 | Bazzi | Mapping the Cold ISM with JWST PAH Emission: The Largest Molecular Cloud Catalog to Date |
| C3 | Caza | Dynamics of Dense Gas Filaments in the Serpens South Star-Forming Region |
| C4 | Cusack | The Fragmentation of Molecular Clouds in Starburst Environments |
| C5 | Dannhauer | The Diamond Ring in Cygnus X – Environment Dictates Bubble Evolution |
| C6 | Green | A large ACA mosaic of 30 Doradus and the connection between its molecular gas and young clusters |
| C7 | Guerrero-Gamboa | The Role of Magnetic Fields in Turbulence Amplification and Gravitational Collapse |
| C8 | Krebs | Millimeter variability of proto-planetary disks |
| C9 | Kobayashi | The impact of multiple supernovae: density and turbulent structures of molecular clouds |
| C10 | Komichi | Study on chemical evolution during molecular cloud formation based on 3-dimensional MHD simulations |
| C11 | Kormann | The Superclouds of the Local Milky Way |
| C12 | Lipman | Central Station: Mass Flow Into and Around the Galactic Center Using Observation and Simulation |
| C13 | Marin | Magnetic Zooms: Testing how magnetic fields shape galaxy structure and star formation |
| C14 | Meingast | Unveiling the Galactic Ice Reservoir: Large-Scale Mapping of Water Ice and Environmental Dependencies in the Ophiuchus star-forming region |
| C15 | Motte | Investigating the origin of stellar masses and the formation of high-mass stars with ALMA-IMF |
| C16 | Najimudeen | BISTRO: Mapping 3D Magnetic Fields in the Milky Way’s Central Molecular Zone |
| C17 | Shahhoseini | Understanding the density PDFs of molecular clouds – the 3D view by Gaia. |
| C18 | Spedicato | Characterizing the fractal dimension of molecular clouds |
| C19 | Suin | A new perspective on pre-supernova feedback, based on high-resolution MHD simulations. |
| C20 | Tharakkal | Synthetic polarisation maps of molecular clouds using magnetohydrodynamic models |
| C21 | Xhemollari | Tracing Internal Clocks in Dense Molecular Clouds via 3D MHD |
| C22 | Zhou | On the millimetre variability of massive proto-stellar sources: First results with GASTON-GP data |
Clusters
| ID | Presenter | Title |
|---|---|---|
| S1 | Allen | The Long-Term Evolution and Dissolution of Young Stellar Clusters |
| S2 | Álvarez-Gutiérrez | N2H+ kinematic analysis of the intermediate protocluster G353.41 |
| S3 | Alves de Oliveira | A New Spectral Class of Brown Dwarfs at the Bottom of the Initial Mass Function in IC 348 |
| S4 | Ballesteros-Paredes | Gravity or turbulence? Stellar kinematics as evidence of molecular cloud dynamics. |
| S5 | Hein | A key to IMF variations at the high-mass end? – The role of stochasticity |
| S6 | Hunt | Unlocking the full potential of the Milky Way's star clusters with their selection function |
| S7 | Hutschenreuter | The velocity field of the Scorpius-Centaurus OB association |
| S8 | Maconi | The Galactic journey of the Solar System in the Gaia era |
| S9 | Pantaleoni González | The 3D map of the solar neighbourhood, using spectroscopically confirmed OB stars and Gaia DR3 |
| S10 | Polnitzky | Precise determination of circumstellar disk lifetimes |
| S11 | Sanchez-Sanjuán | Kinematic analysis and evolution of young stellar clusters in the Orion star-forming complex |
Methods and techniques
| ID | Presenter | Title |
|---|---|---|
| M1 | Crompvoets | Beyond Colour Cuts: Homogenous Methods for Identification of YSOs from any JWST Dataset using Machine Learning |
| M2 | Di Francesco | It's Getting CRISPy in Perseus: New Tools Identify Non-Uniform Velocity Structures in Filaments |
| M3 | Faes | An improved zoom-in method to bridge the scales from global galactic dynamics to local star formation |
| M4 | Gonzalez García | The topology of star-forming regions: clusters and voids |
| M5 | Le Quesne | Fractal Recursive Algorithms and ISM Projections |
| M6 | Niederbrunner | Evaporation Ages: A Revised Dating Technique using Bayesian Modelling |
| M7 | Orjuela López | Machine Learning and Bayesian Inference: Finding Velocity Components of N₂H⁺ in Protocluster G327.29 and Classifying Infrared Spectra of Be Stars. |
| M8 | Pérez Couto | Kinematics of Molecular Clouds: A Comparative Study Using YSOs and Young Open Clusters |