Zobrazeno 1 - 10
of 34
pro vyhledávání: '"Cazzoli, Sara"'
Autor:
Villar-Martin, Montse, Cobá, Carlos López, Cazzoli, Sara, Montero, Enrique Pérez, Lavers, Antonio Cabrera
Publikováno v:
A&A 690, A397 (2024)
Giant (>100 kpc) nebulae associated with active galaxies provide rich information about the circumgalactic medium (CGM) around galaxies, its link with the interstellar medium (ISM) of the hosts and the mechanisms involved in their evolution. We have
Externí odkaz:
http://arxiv.org/abs/2407.02115
Autor:
Mahoro, Antoine, Väisänen, Petri, Pović, Mirjana, Nkundabakura, Pheneas, van der Heyden, Kurt, Cazzoli, Sara, Worku, Samuel B., Márquez, Isabel, Masegosa, Josefa, Randriamampandry, Solohery M., Mogotsi, Moses
We present a study of the $\rm{[OIII]\lambda\,5007}$ line profile in a sub-sample of 8 active galactic nuclei (AGN) and 6 non-AGN in the optically-selected green valley at $\rm{z\,<\,0.5}$ using long-slit spectroscopic observations with the 11 m Sout
Externí odkaz:
http://arxiv.org/abs/2304.09284
Autor:
Muñoz, Laura Hermosa, Márquez, Isabel, Cazzoli, Sara, Masegosa, Josefa, Agís-González, Beatriz
Publikováno v:
A&A 660, A133 (2022)
Outflows play a major role in the evolution of galaxies. However, we do not have yet a complete picture of their properties (extension, geometry, orientation and clumpiness). For low-luminosity Active Galactic Nuclei (AGNs), in particular, low-ionisa
Externí odkaz:
http://arxiv.org/abs/2201.05080
Publikováno v:
RNAAS, 5, 198 (2021)
We present Gemini/NIFS near-IR integral field spectroscopy of the fields-of-view around two AGNs behind the Fermi Bubbles (PDS 456 and 1H1613-097) to search for molecular gas in the Milky Way's nuclear wind. These two AGN sightlines were selected by
Externí odkaz:
http://arxiv.org/abs/2108.11958
Autor:
Saturni, Francesco Gabriele, Vietri, Giustina, Piconcelli, Enrico, Vignali, Christian, Bischetti, Manuela, Bongiorno, Angela, Cazzoli, Sara, Feruglio, Chiara, Fiore, Fabrizio, Husemann, Bernd, Almeida, Cristina Ramos
Publikováno v:
A&A 654, A154 (2021)
The most accepted scenario for the evolution of massive galaxies across cosmic time predicts a regulation based on the interplay between AGN feedback, which injects large amounts of energy in the host environment, and galaxy mergers, being able to tr
Externí odkaz:
http://arxiv.org/abs/2107.12242
Autor:
González-Alfonso, Eduardo, Pereira-Santaella, Miguel, Fischer, Jacqueline, García-Burillo, Santiago, Yang, Chentao, Alonso-Herrero, Almudena, Colina, Luis, Ashby, Matthew L. N., Smith, Howard A., Rico-Villas, Fernando, Martín-Pintado, Jesús, Cazzoli, Sara, Stewart, Kenneth P.
Publikováno v:
A&A 645, A49 (2021)
Galaxies with nuclear bars are believed to efficiently drive gas inward, generating a nuclear starburst and possibly an active galactic nucleus (AGN). We confirm this scenario for the isolated, double-barred, luminous infrared galaxy ESO 320-G030 bas
Externí odkaz:
http://arxiv.org/abs/2011.00347
Autor:
Fox, Andrew J., Ashley, Trisha, Benjamin, Robert A., Bland-Hawthorn, Joss, Bordoloi, Rongmon, Cazzoli, Sara, Hernandez, Svea S., Karim, Tanveer, Jenkins, Edward B., Lockman, Felix J., Kim, Tae-Sun, Wakker, Bart P.
Two giant plasma lobes, known as the Fermi Bubbles, extend 10 kpc above and below the Galactic Center. Since their discovery in X-rays in 2003 (and in gamma-rays in 2010), the Bubbles have been recognized as a new morphological feature of our Galaxy
Externí odkaz:
http://arxiv.org/abs/1903.04833
Autor:
Pereira-Santaella, Miguel, Alonso-Herrero, Almudena, Colina, Luis, Miralles-Caballero, Daniel, Pérez-González, Pablo G., Arribas, Santiago, Bellocchi, Enrica, Cazzoli, Sara, Díaz-Santos, Tanio, López, Javier Piqueras
Publikováno v:
A&A 577, A78 (2015)
We present the analysis of the integrated spectral energy distribution (SED) from the ultraviolet (UV) to the far-infrared and H$\alpha$ of a sample of 29 local systems and individual galaxies with infrared (IR) luminosities between 10^11 Lsun and 10
Externí odkaz:
http://arxiv.org/abs/1502.07965
Autor:
Hermosa Muñoz, Laura, Márquez, Isabel, Cazzoli, Sara, Masegosa, Josefa, Agís-González, Beatriz
Outflows play a major role in the evolution of galaxies and are said to be ubiquitous within the Active Galactic Nuclei (AGNs) population. However, we are far from having a complete picture of their properties, specially considering their impact on t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0bdd9b026ea9cbf9101c1eefff03af5b
Autor:
Molina, Borja Montoro, Guerrero, M.A., Pérez-Díaz, B., J.A.Toalá, Cazzoli, Sara, Bertolami, M.M Miller, Morisset, C.
HuBi 1 is the latest addition to the small but potentially not-so-strange group of born-again planetary nebulae. The VLTP suffered by its central star attenuated its magnitude by 10 mag in just 50 years, as well as giving it a unique inverted ionizat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::242521411ece70e76d4e99f2b0868def