Ghent University Academic Bibliography

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Towards an observationally motivated AGN dusty torus model : II. The roles of density distribution and chemical composition of the dust

Omar Ulises Reyes-Amador, Omaira González-Martín, Jacopo Fritz, Maarten Baes (UGent) , Sundar Srinivasan, Ismael García-Bernete, Donaji Esparza-Arredondo and Marko Stalevski (UGent)

(2025) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 543(1). p.813-840
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Towards an observationally motivated AGN dusty torus model : I. Dust chemical composition from the modelling of Spitzer spectra

Omar Ulises Reyes-Amador, Jacopo Fritz, Omaira González-Martín, Sundar Srinivasan, Maarten Baes (UGent) , Enrique Lopez-Rodriguez, Natalia Osorio-Clavijo, Cesar Iván Victoria-Ceballos, Marko Stalevski (UGent) and C Ramos Almeida

(2024) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 531(1). p.1841-1855
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The role of grain size in active galactic nuclei torus dust models

Omaira González-Martín, Cristina Ramos Almeida, Jacopo Fritz (UGent) , Almudena Alonso-Herrero, Sebastian F. Hönig, Patrick F. Roche, Donaji Esparza-Arredondo, Ismael García-Bernete, Santiago García-Burillo, Natalia Osorio-Clavijo, et al.

(2023) ASTRONOMY & ASTROPHYSICS. 676.
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X-ray nuclear activity in S⁴G barred galaxies : no link between bar strength and co-occurrent supermassive black hole fueling

Mauricio Cisternas, Dimitri A Gadotti, Johan H Knapen, Taehyun Kim, Simon Diaz-Garcia, Eija Laurikainen, Heikki Salo, Omaira Gonzalez-Martin, Luis C Ho, Bruce G Elmegreen, et al.

(2013) ASTROPHYSICAL JOURNAL. 776(1).

Academic Bibliography

Towards an observationally motivated AGN dusty torus model : II. The roles of density distribution and chemical composition of the dust

Towards an observationally motivated AGN dusty torus model : I. Dust chemical composition from the modelling of Spitzer spectra

The role of grain size in active galactic nuclei torus dust models

X-ray nuclear activity in S⁴G barred galaxies : no link between bar strength and co-occurrent supermassive black hole fueling

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