Imagen de Portada

Why are optical coronal lines faint in active galactic nuclei?

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	McKaig, Jeffrey D., Satyapal, Shobita, Laor, Ari, Abel, Nicholas P., Doan, Sara M., Ricci, Claudio, Cann, Jenna M.
Formato:	Preprint
Publicado:	2024
Materias:	Astrophysics of Galaxies High Energy Astrophysical Phenomena
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

The CLASS Quasar Catalog: Coronal Line Activity in Type 1 SDSS Quasars
por: Doan, Sara, et al.
Publicado: (2025)

An Increase in the Prevalence of Ionized Outflows in Galaxies with Coronal Line Emission: Feedback in Action?
por: Matzko, William, et al.
Publicado: (2025)

AGN versus Star-formation: A MUSE Analysis of NGC 1365
por: Mullaney, Kyla, et al.
Publicado: (2026)

Effective & Ethical Mentorship in Physics and Astronomy through Grassroots Organizations
por: Latouf, Natasha, et al.
Publicado: (2024)

Galaxy evolution in the post-merger regime. III -- The triggering of active galactic nuclei peaks immediately after coalescence
por: Ellison, Sara L., et al.
Publicado: (2024)

Local Analogs of Primordial Galaxies: In Search of Intermediate Mass Black Holes with JWST NIRSpec
por: Doan, Sara, et al.
Publicado: (2024)

Investigating the interplay between the coronal properties and the hard X-ray variability of active galactic nuclei with NuSTAR
por: Serafinelli, Roberto, et al.
Publicado: (2024)

The miniJPAS Survey: The radial distribution of star formation rates in faint X-ray active galactic nuclei
por: Acharya, Nischal, et al.
Publicado: (2024)

Population synthesis of active galactic nuclei based on the radiation-regulated unification model
por: Gerolymatou, D., et al.
Publicado: (2026)

A closer look at dwarf galaxies exhibiting MIR variability: AGN confirmation and comparison with non-variable dwarf galaxies
por: Aravindan, Archana, et al.
Publicado: (2024)

The optical-infrared relation for active galactic nuclei: The role of contaminations
por: Rałowski, Mateusz, et al.
Publicado: (2026)

How can the optical variation properties of active galactic nuclei be unbiasedly measured?
por: Hu, Xu-Fan, et al.
Publicado: (2023)

High frequency breaks in optical active galactic nuclei power spectral density
por: Yuk, Heechan, et al.
Publicado: (2023)

Selection of optically variable active galactic nuclei via a random forest algorithm
por: De Cicco, Demetra, et al.
Publicado: (2025)

Spectral indices in active galactic nuclei as seen by Apertif and LOFAR
por: Kutkin, A. M., et al.
Publicado: (2025)

The limits of feedback from active galactic nuclei
por: Pontzen, Andrew, et al.
Publicado: (2026)

Scavenger hunt: Selection of obscured active galactic nuclei combining multiband optical variability and colors
por: De Cicco, Demetra, et al.
Publicado: (2026)

Broadband X-ray/UV/optical time-resolved spectroscopy of NGC 5548: The origin of the UV/optical variability in active galactic nuclei
por: Kammoun, E., et al.
Publicado: (2024)

Collisions of red giants in galactic nuclei
por: Ryu, Taeho, et al.
Publicado: (2023)

Polarization of active galactic nuclei with significant VLBI-Gaia displacements
por: Blinov, Dmitry, et al.
Publicado: (2024)

Euclid preparation. Spectroscopy of active galactic nuclei with NISP
por: Euclid Collaboration, et al.
Publicado: (2023)

Investigating the nuclear properties of highly accreting active galactic nuclei with XMM-Newton
por: Laurenti, M., et al.
Publicado: (2024)

Formation of dust clumps in the torus of active galactic nuclei
por: Cao, Xinwu, et al.
Publicado: (2026)

The role of bars in triggering active galactic nuclei galaxies
por: Marels, V., et al.
Publicado: (2025)

Population III star formation near high-redshift active galactic nuclei
por: Fisk, Ethan M., et al.
Publicado: (2025)

The size-luminosity relation of local active galactic nuclei from interferometric observations of the broad-line region
por: GRAVITY Collaboration, et al.
Publicado: (2024)

BASS. XLIII: Optical, UV, and X-ray emission properties of unobscured Swift/BAT active galactic nuclei
por: Gupta, Kriti K., et al.
Publicado: (2024)

On joint analysing XMM-NuSTAR spectra of active galactic nuclei
por: Kang, Jia-Lai, et al.
Publicado: (2023)

CAZ catalog and optical light curves of 7918 blazar-selected active galactic nuclei
por: Kouch, Pouya M., et al.
Publicado: (2025)

Properties of black hole mergers in disks of active galactic nuclei
por: Tagawa, Hiromichi, et al.
Publicado: (2026)

Multi-wavelength properties of changing-state active galactic nuclei: I. the evolution of soft excess and X-ray continuum
por: Jana, Arghajit, et al.
Publicado: (2026)

The relation between the optical variability timescale, magnetic field of jets and black hole spin in active galactic nuclei
por: Chen, Yongyun, et al.
Publicado: (2025)

On the transformation of the Maxwell-Boltzmann Distribution to a Power-Law
por: Laor, Ari, et al.
Publicado: (2026)

The cold molecular gas regulates the activity of active galactic nuclei in massive galaxies
por: Chen, Yongyun, et al.
Publicado: (2026)

EMU/GAMA: A statistical perspective on active galactic nuclei diagnostics
por: Prathap, J., et al.
Publicado: (2026)

Quasi-periodic oscillations in optical color evolutions to support sub-pc binary black hole systems in broad line active galactic nuclei
por: XueGuang, Zhang
Publicado: (2025)

Unveiling the quasar main sequence: illuminating the complexity of active galactic nuclei and their evolution
por: Panda, Swayamtrupta
Publicado: (2024)

The variability angular diameter distance and the intrinsic brightness temperature of active galactic nuclei
por: Cheong, Whee Yeon, et al.
Publicado: (2025)

Connecting outflows with radio emission in active galactic nuclei at cosmic noon
por: Ilha, Gabriele S., et al.
Publicado: (2025)

Hidden No More: Spotlight on tidal disruption events in active galactic nuclei
por: Veres, Patrik Milán
Publicado: (2025)