| Almendros-Abad |
The substellar population of massive young clusters with JWST |
| Alves |
Massive stars form complexes of pc-scale filaments |
| Audard |
Identifying time-variable young stars in the Milky Way with Big Data |
| Barnes |
The Phantom Void: Connecting Feedback, Star Formation, and Superbubble Evolution from Nearby Galaxies to the Milky Way |
| Bernard |
Dawn: The genesis and early evolution of embedded clusters |
| Böhm |
Feeding the Stellar Nursery: Accretion and Feedback Processes in W33 Main |
| Bonanomi |
Turbulence dissipation and the formation of dense fibers |
| Bosomworth |
Resolved Dust Emission and CO Isotopologues in Giant Molecular Clouds of the Andromeda Galaxy |
| Budaiev |
Multiwavelength mysteries in the most star-forming cloud in the Galactic center |
| Chevalier |
Extracting virialized structures in numerical simulations |
| Clark |
Disentangling galactic-scale CO emission |
| Dalcanton |
Large Area HST Surveys of Star-Forming Galaxies in the Local Group |
| Daugevičius |
Mass Function of Star Clusters in the M31 Disc |
| do Brito do Vale |
Stellar population of the young cluster RCW 36 in Vela |
| Dumond |
A mass invariant in the compressible gravoturbulent ISM |
| Eibensteiner |
Molecular Gas Fraction and Dynamical Equilibrium Pressure in Local and Nearby Galaxies |
| Forbrich |
The Orion Radio All-Stars: Probing Extreme Space Weather in Young Stellar Objects |
| Fuller |
The Multi-scale structure of magnetic fields, gravity, and turbulence in massive star formation: The STREAMS project |
| Heigl |
Getting to the core: Bonnor-Ebert spheres drive non-linear collapse in filaments |
| Houghton |
The star formation rate in the Central Molecular Zone of the Milky Way using JWST imaging |
| Jimenez-Donaire |
Key signatures of molecular gas: linking dense gas and star formation across a diverse set of environments |
| Kainulainen |
Molecular cloud morphology revisited: a machine learning approach to identifying key properties |
| Kashiwagi |
Exploring Fundamental Evolutionary Processes of Filament-Filament Collisions: Toward Understanding the Hub-Filament Paradigm |
| Ksoll |
How to Solve Inverse Problems in Astronomy with Invertible Neural Networks |
| Liang |
Modeling the multi-phase ISM shaped by star formation and feedback in the LMC |
| Mercimek |
Mass accretion and ejection phenomena in chemically rich filaments and outflows of high-mass star-forming objects: the ALMA SQUALO project |
| Miller |
The Driving Mode of Turbulence in Extragalactic Sources |
| Nakamura |
Turbulence or Gravity? Deciphering the Origin of Dense Cores in Molecular Clouds |
| Negueruela |
It doesn't work as we thought! The Outer Milky Way forms large dispersed star complexes |
| Neupane |
High resolution APEX/LAsMA observations of 12CO and 13CO J = 3 - 2 toward the NGC 6334 extended filament |
| Nucara |
The Rosetta Stone project: a self-consistent simulation-to-observation study of massive star-forming clumps |
| Ossenkopf-Okada |
How to feed star formation? The carbon puzzle |
| Patel |
Identification and Characterization of Filaments in Simulated Molecular Clouds |
| Posch |
Chains of clusters in Sco-Cen: Tracing cloud acceleration driven by stellar feedback |
| Priestley |
Molecular line tracers of dense gas, `dense' gas, and the star formation rate |
| Quintana |
A new Gaia census of OB associations within 1 kpc |
| Ratzenboeck |
Learning with Gaps: A Domain-Adaptive ML Framework for Mapping Young Stars from Incomplete, Multi-Survey Data |
| Romanelli |
Environmental dependance of GMC evolution and star formation in nearby galaxies |
| Rygl |
Initial stages of star cluster formation in the W48 star-forming complex |
| Sandoval |
N2H+ kinematic analysis in G351.77: Initial conditions and evolution of a massive protocluster. |
| Santos Do Amaral |
Towards a statistical characterization of the earliest stages of high-mass star formation |
| Schisano |
How do clustered systems form? Clues on the beginning and temporal progress of the fragmentation process from the spatial distribution of dense star-forming cores in the ALMAGAL survey |
| Seifried |
MHD simulations of molecular clouds and synthetic dust polarisation maps: What can we learn from it? |
| Socci |
Fiber networks in Orion: star formation and width variations |
| Soler |
The large-scale environment of local star formation: physical conditions of the diffuse gas in the Solar Neighborhood |
| Steffes |
Measuring Velocity Gradients of Gas into Filament Spines and Prestellar Cores in the Taurus Molecular Cloud |
| Swiggum |
Rewinding 70 million years of nearby Star Formation with Gaia |
| Tafalla |
Characterizing the emission of molecular clouds using a sampling technique |
| Thompson |
HII regions from big to small with MeerKAT and the JVLA |
| Tsuge |
High-mass star formation in the Large Magellanic Cloud triggered by colliding HI flows |
| Wells |
From theory to observation: understanding filamentary flows in high-mass star-forming clusters |
| Williams |
ALMA spatial filtering responsible for shallowing the slopes of core mass functions (CMFs) in distant clouds |
| Xu |
Dynamic view of massive protocluster formation |
| Yoo |
ALMA/JWST view of W51-E and W51-IRS2 protoclusters |
| Zari |
The large-scale kinematics of young stars in the Milky Way disc: first results from SDSS-V |
| Zhang |
Magnetic fields and massive protoclusters |
