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pro vyhledávání: '"Almeyda, Triana"'
The variable continuum emission of an active galactic nucleus (AGN) produces corresponding responses in the broad emission lines, which are modulated by light travel delays, and contain information on the physical properties, structure, and kinematic
Externí odkaz:
http://arxiv.org/abs/2311.03590
A galaxy merger is expected to cause the formation of a supermassive black hole (SMBH) binary, which itself eventually coalesces through the anisotropic emission of gravitational waves. This may result in the merged SMBH receiving a recoil kick veloc
Externí odkaz:
http://arxiv.org/abs/2107.14711
The size and structure of the dusty circumnuclear torus in active galactic nuclei (AGN) can be investigated by analyzing the temporal response of the torus's infrared (IR) dust emission to variations in the AGN ultraviolet/optical luminosity. This me
Externí odkaz:
http://arxiv.org/abs/2002.12823
Akademický článek
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The obscuring circumnuclear torus of dusty molecular gas is one of the major components of active galactic nuclei (AGN). The torus can be studied by analyzing the time response of its infrared (IR) dust emission to variations in the AGN continuum lum
Externí odkaz:
http://arxiv.org/abs/1709.07011
Autor:
Vazquez, Billy, Galianni, Pasquale, Richmond, Michael, Robinson, Andrew, Axon, David J., Horne, Keith, Almeyda, Triana, Fausnaugh, Michael, Peterson, Bradley M., Bottorff, Mark, Gallimore, Jack, Eltizur, Moshe, Netzer, Hagai, Storchi-Bergmann, Thaisa, Marconi, Alessandro, Capetti, Alessandro, Batcheldor, Dan, Buchanan, Catherine, Stirpe, Giovanna, Kishimoto, Makoto, Packham, Christopher, Perez, Enrique, Tadhunter, Clive, Upton, John, Estrada-Carpenter, Vicente
We present results from a fifteen-month campaign of high-cadence (~ 3 days) mid-infrared Spitzer and optical (B and V ) monitoring of the Seyfert 1 galaxy NGC 6418, with the objective of determining the characteristic size of the dusty torus in this
Externí odkaz:
http://arxiv.org/abs/1502.01977
Autor:
Almeyda, Triana
The obscuring circum-nuclear dusty torus is a major component of AGN and yet, thus far, its shape, composition, and structure have not been well constrained by observations. However, using indirect methods such as reverberation mapping, the size and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::580ab465561021a3c7a112533f77291a