Imagen de Portada

The excess of molecular hydrogen in chemical networks without oxygen

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autor principal:	Ploeckinger, Sylvia
Formato:	Preprint
Publicado:	2025
Materias:	Astrophysics of Galaxies
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Resolution criteria to avoid artificial clumping in Lagrangian hydrodynamic simulations with a multi-phase interstellar medium
por: Ploeckinger, Sylvia, et al.
Publicado: (2023)

A subgrid model for chemical enrichment in cosmological simulations
por: Correa, Camila A., et al.
Publicado: (2026)

The importance of super-Eddington black hole accretion for the emergence of massive quiescent galaxies at high redshift
por: Chaikin, Evgenii, et al.
Publicado: (2026)

TangoSIDM Project: Is the Stellar Mass Tully-Fisher relation consistent with SIDM?
por: Correa, Camila, et al.
Publicado: (2024)

Hybrid-chimes: A model for radiative cooling and the abundances of ions and molecules in simulations of galaxy formation
por: Ploeckinger, Sylvia, et al.
Publicado: (2025)

Modeling molecular hydrogen in low metallicity galaxies
por: Polzin, Ava, et al.
Publicado: (2023)

Low-ionization structures in planetary nebulae -- IV. The molecular hydrogen counterpart
por: Mari, M. B., et al.
Publicado: (2025)

Turning JWST/MIRI backgrounds into a survey of diffuse molecular hydrogen
por: Nigou, E., et al.
Publicado: (2026)

A model for molecular hydrogen-dependent star formation in simulations of galaxy evolution
por: Lozano, Ezequiel, et al.
Publicado: (2023)

Exploring the chemical evolution in hot molecular cores
por: Martinez, N. C., et al.
Publicado: (2026)

A hybrid active galactic nucleus feedback model with spinning black holes, winds and jets
por: Huško, Filip, et al.
Publicado: (2025)

LYRA ultra-faints: The emergence of faint dwarf galaxies in the presence of an early Lyman-Werner background
por: Brown, Shaun T., et al.
Publicado: (2025)

Detection of a molecular hydrogen envelope around nova GK Persei
por: Banerjee, D. P. K., et al.
Publicado: (2026)

Hydroxylated Mg-rich amorphous silicates as catalysts for molecular hydrogen formation in the interstellar medium
por: Mennella, V., et al.
Publicado: (2025)

Methanimine as a sink in the HCN and HNC solid state hydrogenation network
por: Enrique-Romero, Joan, et al.
Publicado: (2026)

Modelling the evolution and influence of dust in cosmological simulations that include the cold phase of the interstellar medium
por: Trayford, James W., et al.
Publicado: (2025)

Excitation of molecular hydrogen by cosmic-ray protons
por: Padovani, Marco, et al.
Publicado: (2025)

The evolution of the galaxy stellar mass function and star formation rates in the COLIBRE simulations from redshift 17 to 0
por: Chaikin, Evgenii, et al.
Publicado: (2025)

Detection of thioacetaldehyde (CH3CHS) in TMC-1: sulfur-oxygen differentiation along the hydrogenation sequence
por: Agundez, M., et al.
Publicado: (2025)

One hundred optical emission lines of molecular hydrogen from a low-metallicity photodissociation region
por: Henney, William J., et al.
Publicado: (2023)

Complex hydrogen chemical equilibrium and Gaia low mass problem in cool white dwarfs
por: Kowalski, Piotr M.
Publicado: (2026)

Non-explosive pre-supernova feedback in the COLIBRE model of galaxy formation
por: Benítez-Llambay, Alejandro, et al.
Publicado: (2025)

Comparing the morphology of molecular clouds without supervision
por: Richard, Pablo, et al.
Publicado: (2024)

Effect of molecular hydrogen self-shielding modeling on early Reionization Era galaxies in radiative hydrodynamic cosmological simulations
por: Nguyen, Thinh Huu, et al.
Publicado: (2025)

Tracking the dynamical, chemical and spectral evolution of molecular cores with PrestaLine: Gorynych
por: Kochina, Olga, et al.
Publicado: (2026)

Dynamical disequilibrium in dwarf galaxies: rethinking gas dynamics, rotation curves, and dark matter inference
por: Dado, Diego, et al.
Publicado: (2025)

Dwarf Galaxies with Radio-excess AGNs in the VLA Sky Survey
por: Eberhard, John-Michael, et al.
Publicado: (2024)

The impact of attenuation on cosmic-ray chemistry: I. Abundances and chemical calibrators in molecular clouds
por: Roy, Arghyadeb, et al.
Publicado: (2026)

Digging into the chemical complexity in the outer Galaxy: A hot molecular core in Sharpless 2-283
por: Ikeda, Toki, et al.
Publicado: (2026)

Gravitational potential drives the concentration dependence of the stellar mass-halo mass relation
por: Wang, Kai, et al.
Publicado: (2025)

The morphologies of present-day galaxies in the COLIBRE simulations
por: Moreno, Victor J. Forouhar, et al.
Publicado: (2026)

The physical and chemical structure of Sagittarius B2, VIII. Full molecular line survey of hot cores
por: Möller, T., et al.
Publicado: (2024)

No evidence for excess AGN activity in recently quenched massive galaxies at cosmic noon
por: Almaini, Omar, et al.
Publicado: (2025)

Interpretations of galaxy spectra at high redshift. \ The H_gamma/H_beta excess
por: Contini, M.
Publicado: (2026)

Time-dependent chemical evolution during cloud formation: H$_2$-regulated chemistry in diffuse molecular cloud
por: Komichi, Yuto, et al.
Publicado: (2026)

Modelling the multi-wavelength detection of protoclusters. I: An excess of submillimetre galaxies in protocluster cores
por: Araya-Araya, Pablo, et al.
Publicado: (2024)

The EDGES measurement disfavors an excess radio background during the cosmic dawn
por: Cang, Junsong, et al.
Publicado: (2024)

CO emission survey of asymptotic giant branch stars with ultraviolet excesses
por: Alonso-Hernández, Jaime, et al.
Publicado: (2024)

Two faces of Gaia-Sausage-Enceladus: Mining the chemical abundance space with graph attention networks
por: Quandt-Rodriguez, Milan, et al.
Publicado: (2026)

Detection and chemical modelling of complex prebiotic molecule cyanamide in the hot molecular core G31.41+0.31
por: Manna, Arijit, et al.
Publicado: (2024)