Imagen de Portada

Radiative and mechanical energies in galaxies I. Contributions of molecular shocks and PDRs in 3C 326 N

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Villa-Vélez, J. A., Godard, B., Guillard, P., Forêts, G. Pineau des
Formato:	Preprint
Publicado:	2024
Materias:	Astrophysics of Galaxies
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

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

Shocks in the warm neutral medium I -- Theoretical model
por: Godard, Benjamin, et al.
Publicado: (2024)

Shocks in the warm neutral medium II -- Origin of neutral carbon at high pressure
por: Godard, Benjamin, et al.
Publicado: (2024)

Physical conditions in Centaurus A's northern filaments II: Does the HCO$^+$ emission highlight the presence of shocks?
por: Salomé, Quentin, et al.
Publicado: (2024)

JWST imaging of the Pleiades: anisotropy of turbulence in the cold neutral medium
por: Vigoureux, G., et al.
Publicado: (2026)

JWST/NIRSpec and MIRI observations of an expanding, jet-driven bubble of warm H$_2$ in the radio galaxy 3C 326 N
por: Leftley, James H., et al.
Publicado: (2024)

PDRs4All XV: CH radical and H$_3^+$ molecular ion in the irradiated protoplanetary disk d203-506
por: Schroetter, I., et al.
Publicado: (2025)

PDRs4All VII. The 3.3 $μ$m aromatic infrared band as a tracer of physical properties of the ISM in galaxies
por: Schroetter, Ilane, et al.
Publicado: (2024)

Velocity-resolved [O I] 63,145 um, [C II] 158 um, and OH mapping along the Orion BN/KL explosive outflow and irradiated shocks
por: Goicoechea, J. R., et al.
Publicado: (2026)

PDRs4All IX. Sulfur elemental abundance in the Orion Bar
por: Fuente, Asunción, et al.
Publicado: (2024)

PDRs4All III: JWST's NIR spectroscopic view of the Orion Bar
por: Peeters, Els, et al.
Publicado: (2023)

PDRs4All. XII. FUV-driven formation of hydrocarbon radicals and their relation with PAHs
por: Goicoechea, J. R., et al.
Publicado: (2025)

PDRs4All II: JWST's NIR and MIR imaging view of the Orion Nebula
por: Habart, Emilie, et al.
Publicado: (2023)

PDRs4All VIII: Mid-IR emission line inventory of the Orion Bar
por: Van De Putte, Dries, et al.
Publicado: (2024)

PDRs4All VI: Probing the Photochemical Evolution of PAHs in the Orion Bar Using Machine Learning Techniques
por: Pasquini, S., et al.
Publicado: (2023)

PDRs4All. V. Modelling the dust evolution across the illuminated edge of the Orion Bar
por: Elyajouri, M., et al.
Publicado: (2024)

PDRs4All IV. An embarrassment of riches: Aromatic infrared bands in the Orion Bar
por: Chown, Ryan, et al.
Publicado: (2023)

Two intersecting radio shells: relics of galaxy merger shocks ?
por: Koribalski, Bärbel S., et al.
Publicado: (2025)

Resolved molecular gas and star-formation in massive unquenched spirals : I. UGC 8179
por: Cologni, Romane, et al.
Publicado: (2026)

PDRs4All XVIII. JWST-NIRCam Photometric properties of protoplanetary disks in the Orion Nebula Cluster
por: Amiot, P., et al.
Publicado: (2026)

PDRs4All XVII: Formation and excitation of HD in photodissociation regions. Application to the Orion Bar
por: Zannese, Marion, et al.
Publicado: (2025)

Central molecular zones in galaxies: 13CO(6-5) and molecular gas conditions in bright nearby galaxies
por: Israel, F. P., et al.
Publicado: (2024)

PDRs4All XI. Detection of infrared CH$^+$ and CH$_3^+$ rovibrational emission in the Orion Bar and disk d203-506: evidence of chemical pumping
por: Zannese, Marion, et al.
Publicado: (2025)

Two distinct molecular cloud populations detected in massive galaxies
por: Rose, Tom, et al.
Publicado: (2024)

PDRs4All XVI. Tracing aromatic infrared band characteristics in photodissociation region spectra with PAHFIT in the JWST era
por: Van De Putte, Dries, et al.
Publicado: (2025)

PDRs4All XIII. Empirical prescriptions for the interpretation of JWST imaging observations of star-forming regions
por: Chown, Ryan, et al.
Publicado: (2024)

PDRs4All: XVIII. The evolution of the PAH ionisation and PAH size distribution across the Orion Bar
por: Maragkoudakis, Alexandros, et al.
Publicado: (2026)

Radiation hydrodynamic simulation of the Haro 11 galaxy: the escape of LyC and Ly$α$ in a dwarf galaxy merger
por: Ejdetjärn, Timmy, et al.
Publicado: (2026)

Large molecular and dust reservoir of a gravitationally-lensed submillimeter galaxy behind the Lupus-I molecular cloud
por: Tamura, Yoichi, et al.
Publicado: (2025)

PDRs4All XIX. The 6 to 9 $μ$m region as a probe of PAH charge and size in the Orion Bar
por: Khan, Baria, et al.
Publicado: (2025)

Empirical instability strip for classical Cepheids: I. The LMC galaxy
por: Espinoza-Arancibia, F., et al.
Publicado: (2023)

X-shaped radio galaxy 3C 315
por: Jovanović, V. Borka, et al.
Publicado: (2025)

What drives the corpulence of galaxies? I. The formation of central compact dwarf galaxies in TNG50
por: De Almeida, Abhner P., et al.
Publicado: (2024)

Radiation-driven dusty outflows from early galaxies
por: Nakazato, Yurina, et al.
Publicado: (2024)

The shocking features in the closest rich galaxy cluster Norma
por: Ge, Chong, et al.
Publicado: (2026)

Augmenting the power of time-delay cosmography in lens galaxy clusters by probing their member galaxies I. Type Ia supernovae
por: Acebron, A., et al.
Publicado: (2023)

Quantitative analysis of the molecular gas morphology in nearby disk galaxies
por: Yamamoto, Takashi, et al.
Publicado: (2024)

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

Supernova Shocks in Molecular Clouds: Shocks Driven into Dense Cores in IC 443 and 3C 391
por: Reach, William T., et al.
Publicado: (2024)

Decomposing the growth mechanisms of galaxies over the last 10 billion years
por: Davies, Luke J. M., et al.
Publicado: (2026)