Zobrazeno 1 - 10
of 595
pro vyhledávání: '"MASEGOSA, J"'
Autor:
Cazzoli, S., Hernández-García, L., Márquez, I., Masegosa, J., Bruni, G., Panessa, F., Bassani, L.
Some giant radio galaxies selected at X-rays with an AGN show signs of a restarted nuclear activity. One object in this peculiar class is Mrk1498, a giant low-frequency double radio source that shows extended emission in [OIII]. This emission is like
Externí odkaz:
http://arxiv.org/abs/2409.07534
Autor:
Muñoz, L. Hermosa, Cazzoli, S., Márquez, I., Masegosa, J., Chamorro-Cazorla, M., de Paz, A. Gil, Castillo-Morales, Á., Gallego, J., Carrasco, E., Iglesias-Páramo, J., García-Vargas, M. L., Gómez-Álvarez, P., Pascual, S., Pérez-Calpena, A., Cardiel, N.
Publikováno v:
A&A 683, A43 (2024)
Outflows are believed to be ubiquitous in all AGNs, although their presence in low luminosity AGNs, in particular, for LINERs, has only started to be explored. Their properties (geometry, mass and energetics) are still far from being properly charact
Externí odkaz:
http://arxiv.org/abs/2311.12552
Autor:
Cazzoli, S., Muñoz, L. Hermosa, Márquez, I., Masegosa, J., Castillo-Morales, A., de Paz, A. Gil, Hernández-García, L., La Franca, F., Almeida, C. Ramos
Outflows play a central role in galaxy evolution shaping the properties of galaxies. Understanding outflows and their effects in low luminosity AGNs, such as LINERs, is essential (e.g. they are a numerous AGN population in the local Universe). We obt
Externí odkaz:
http://arxiv.org/abs/2204.02416
The morphological classification of active galaxies may be affected by the presence of active galactic nuclei (AGN). In this paper, we provide the most detailed analysis on how different AGN contributions, from 5% to 75%, to the total optical light m
Externí odkaz:
http://arxiv.org/abs/2203.07702
Autor:
Martínez-Paredes, M., González-Martín, O., HyeongHan, K., Geier, S., García-Bernete, I., Almeida, C. Ramos, Alonso-Herrero, A., Aretxaga, I., Kim, M., Sohn, B. W., Masegosa, J.
To study the nuclear ($\lesssim1\,$kpc) dust of nearby ($z<0.1$) type 1 Quasi Stellar Objects (QSOs) we obtained new near-infrared (NIR) high angular resolution ($\sim0.3$ arcsec) photometry in the H and Ks bands, for 13 QSOs with available mid-infra
Externí odkaz:
http://arxiv.org/abs/2108.08043
Autor:
del Moral-Castro, I., García-Lorenzo, B., Almeida, C. Ramos, Ruiz-Lara, T., Falcón-Barroso, J., Sánchez, S. F., Sánchez-Blázquez, P., Márquez, I., Masegosa, J.
Publikováno v:
A&A 639, L9 (2020)
We present a comparison of the spin parameter $\lambda_R$, measured in a region dominated by the galaxy disc, between 20 pairs of nearby (0.005$<$z$<$0.03) seemingly isolated twin galaxies differing in nuclear activity. We find that 80--82% of the ac
Externí odkaz:
http://arxiv.org/abs/2006.12654
Autor:
Cazzoli, S., Márquez, I., Masegosa, J., del Olmo, A., Povic, M., González-Martín, O., Balmaverde, B., Hernández-García, L., García-Burillo, S.
Publikováno v:
Proceedings of the International Astronomical Union (356), 2019. Eds. M. Povic, J. Masegosa, H. Netzer, P. Marziani, P. Shastri, S. B. Tessema & S. H. Negu
We present the highlights from our recent study of 22 local (z$<$0.025) type-1 LINERs from the Palomar Survey, on the basis of optical long-slit spectroscopic observations taken with TWIN/CAHA, ALFOSC/NOT and HST/STIS (Cazzoli et al. 2018). Our goals
Externí odkaz:
http://arxiv.org/abs/2002.11139
Low-Ionisation Nuclear Emission-line Regions (LINERs) are the least luminous and the most numerous among the local population of Active Galactic Nuclei (AGN). They can be classified as type-1 or type-2 if their optical spectra show or do not show, re
Externí odkaz:
http://arxiv.org/abs/2002.10500
Autor:
Cazzoli, S., de Paz, A. Gil, Márquez, I., Masegosa, J., Iglesias, J., Gallego, J., Carrasco, E., Cedazo, R., García-Vargas, M. L., Castillo-Morales, Á., Pascual, S., Cardiel, N., Pérez-Calpena, A., Gómez-Alvarez, P., Martínez-Delgado, I., Hermosa-Muñoz, L.
We present our analysis of high-resolution (R $\sim$ 20 000) GTC/MEGARA integral-field unit spectroscopic observations, obtained during the commissioning run, in the inner region (12.5 arcsec x 11.3 arcsec) of the active galaxy NGC7469, at spatial sc
Externí odkaz:
http://arxiv.org/abs/2002.04031
Autor:
González-Martín, O., Masegosa, J., García-Bernete, I., Almeida, C. Ramos, Rodríguez-Espinosa, J. M., Márquez, I., Esparza-Arredondo, D., Osorio-Clavijo, N., Martínez-Paredes, M., Victoria-Ceballos, C., Pasetto, A., Dultzin, D.
This is the second in a series of papers devoted to explore a set of six dusty models of active galactic nuclei (AGN) with available spectral energy distributions (SEDs). These models are the smooth torus by Fritz et al. (2006), the clumpy torus by N
Externí odkaz:
http://arxiv.org/abs/1908.11389