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Origin of compressive turbulence in protoclumps in high redshift disks
Omry Ginzburg, Avishai Dekel, Nir Mandelker, Dhruba Dutta Chowdhury, Frederic Bournaud, Daniel Ceverino and Joel Primack Astronomy & Astrophysics 698 A110 (2025) https://doi.org/10.1051/0004-6361/202553729
An Investigation of Disk Thickness in M51 from Hα, Paα, and Mid-infrared Power Spectra
Bruce G. Elmegreen, Daniela Calzetti, Angela Adamo, Karin Sandstrom, Daniel Dale, Varun Bajaj, Martha L. Boyer, Ana Duarte-Cabral, Ryan Chown, Matteo Correnti, Julianne J. Dalcanton, Bruce T. Draine, Brandt Gaches, John S. Gallagher, Kathryn Grasha, Benjamin Gregg, Leslie K. Hunt, Kelsey E. Johnson, Robert Kennicutt, Ralf S. Klessen, Adam K. Leroy, Sean Linden, Anna F. McLeod, Matteo Messa, Göran Östlin, et al. The Astrophysical Journal 986(1) 13 (2025) https://doi.org/10.3847/1538-4357/adcee6
Formation of Supersonic Turbulence in the Primordial Star-forming Cloud
Ugo Lebreuilly, Alessio Traficante, Alice Nucara, Ngo-Duy Tung, Patrick Hennebelle, Sergio Molinari, Ralf S. Klessen, Leonardo Testi, Veli-Matti Pelkonen, Milena Benedettini, Alessandro Coletta, Davide Elia, Chiara Mininni, Stefania Pezzuto, Juan D. Soler, Paolo Suin and Claudia Toci Astronomy & Astrophysics 701 A217 (2025) https://doi.org/10.1051/0004-6361/202554774
Turbulent Gas-rich Disks at High Redshift: Origin of Thick Stellar Disks Through 3D “Baryon Sloshing”
Joss Bland-Hawthorn, Thor Tepper-Garcia, Oscar Agertz, Christoph Federrath, Misha Haywood, Paola di Matteo, Timothy R. Bedding, Takafumi Tsukui, Emily Wisnioski, Melissa Ness and Ken Freeman The Astrophysical Journal 994(1) 22 (2025) https://doi.org/10.3847/1538-4357/ae0931
Clump formation in ram-pressure stripped galaxies: Evidence from mass function
Eric Giunchi, Claudia Scarlata, Ariel Werle, Bianca M. Poggianti, Alessia Moretti, Marco Gullieuszik, Benedetta Vulcani, Alessandro Ignesti, Antonino Marasco, Anita Zanella and Anna Wolter Astronomy & Astrophysics 696 A228 (2025) https://doi.org/10.1051/0004-6361/202452983
The role of the ionizing background on the thermal and non-thermal broadening inferred for the low-z intergalactic O vi absorbers