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  • 1-10 ل  366 نتائج ل ""Institute for Computational Science""
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Academic Journal

The moon-forming impact as a constraint for the inner Solar system’s formation

Subjects: Institute for Computational Science; 530 Physics

  • Source: Fang, Tong; Bi, Rongxi; Zhang, Hui; Zhou, You; Reinhardt, Christian; Deng, Hongping (2025). The moon-forming impact as a constraint for the inner Solar system’s formation. Monthly Notices of the

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Academic Journal

Determining the baryon impact on the matter power spectrum with galaxy clusters

Subjects: Institute for Computational Science; 530 Physics

  • Source: Grandis, Sebastian; Aricò, Giovanni; Schneider, Aurel; Linke, Laila (2024). Determining the baryon impact on the matter power spectrum with galaxy clusters. Monthly Notices of the Royal Astronomical

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Academic Journal

The 21-cm signal during the end stages of reionization

Subjects: Institute for Computational Science; 530 Physics

  • Source: Giri, Sambit K; Bianco, Michele; Schaeffer, Timothée; Iliev, Ilian T; Mellema, Garrelt; Schneider, Aurel (2024). The 21-cm signal during the end stages of reionization. Monthly Notices of the Royal

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Academic Journal

Measuring eccentricity and gas-induced perturbation from gravitational waves of LISA massive black hole binaries

Subjects: Institute for Computational Science; 530 Physics

  • Source: Garg, Mudit; Derdzinski, Andrea; Tiwari, Shubhanshu; Gair, Jonathan; Mayer, Lucio (2024). Measuring eccentricity and gas-induced perturbation from gravitational waves of LISA massive black hole

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Academic Journal

Stellar cluster formation in a Milky Way-sized galaxy at $z > 4$ – II. A hybrid formation scenario for the nuclear star cluster and its connection to the nuclear stellar ring

Subjects: Institute for Computational Science; 530 Physics

  • Source: van Donkelaar, Floor; Mayer, Lucio; Capelo, Pedro R; Tamfal, Tomas; Quinn, Thomas R; Madau, Piero (2024). Stellar cluster formation in a Milky Way-sized galaxy at $z > 4$ – II. A hybrid formation

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Academic Journal

Gas permeability and mechanical properties of dust grain aggregates at hyper- and zero-gravity

Subjects: Institute for Computational Science; 530 Physics

  • Source: Capelo, Holly L; Bodénan, Jean-David; Jutzi, Martin; Kühn, Jonas; Cerubini, Romain; Jost, Bernhard; Stöckli, Linus; Spadaccia, Stefano; Herny, Clemence; Gundlach, Bastian; Kargl, Günter; Surville,

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Academic Journal

TOI-2374 b and TOI-3071 b: two metal-rich sub-Saturns well within the Neptunian desert

Subjects: Institute for Computational Science; 530 Physics

  • Source: Hacker, Alejandro; Díaz, Rodrigo F; Armstrong, David J; Fernández Fernández, Jorge; Müller, Simon; Delgado-Mena, Elisa; Sousa, Sérgio G; Adibekyan, Vardan; Stassun, Keivan G; Collins, Karen A;

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Academic Journal

[C II] 158 μm emission as an indicator of galaxy star formation rate

Subjects: Institute for Computational Science; 530 Physics

  • Source: Liang, Lichen; Feldmann, Robert; Murray, Norman; Narayanan, Desika; Hayward, Christopher C; Anglés-Alcázar, Daniel; Bassini, Luigi; Richings, Alexander J; Faucher-Giguère, Claude-André; Chung,

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Academic Journal

Inflow and outflow properties, not total gas fractions, drive the evolution of the mass–metallicity relation

Subjects: Institute for Computational Science; 530 Physics

  • Source: Bassini, Luigi; Feldmann, Robert; Gensior, Jindra; Faucher-Giguère, Claude-André; Cenci, Elia; Moreno, Jorge; Bernardini, Mauro; Liang, Lichen (2024). Inflow and outflow properties, not total gas

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Academic Journal

Magnetic field amplification in cosmological zoom simulations from dwarf galaxies to galaxy groups

Subjects: Institute for Computational Science; 530 Physics; Space and Planetary Science

  • Source: Pakmor, Rüdiger; Bieri, Rebekka; van de Voort, Freeke; Werhahn, Maria; Fattahi, Azadeh; Guillet, Thomas; Pfrommer, Christoph; Springel, Volker; Talbot, Rosie Y (2024). Magnetic field amplification in

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  • 1-10 ل  366 نتائج ل ""Institute for Computational Science""