Zobrazeno 1 - 10
of 154
pro vyhledávání: '"Delgado, R. González"'
Autor:
Pérez, I., Verley, S., Sánchez-Menguiano, L., Ruiz-Lara, T., García-Benito, R., Puertas, S. Duarte, Jiménez, A., Domínguez-Gómez, J., Espada, D., Peletier, R. F., Román, J., Rodríguez, M. I., Alarcón, P. Sánchez, Argudo-Fernández, M., Torres-Ríos, G., Bidaran, B., Alcázar-Laynez, M., van de Weygaert, R., Sánchez, S. F., Lisenfeld, U., Zurita, A., Florido, E., van der Hulst, J. M., Blázquez-Calero, G., Villalba-González, P., del Moral-Castro, I., Lugo-Aranda, A., Walo-Martín, D., Conrado, A., Delgado, R. González, Falcón-Barroso, J., Ferré-Mateu, A., Hernández-Sánchez, M., Awad, P., Kreckel, K., Courtois, H., Espada-Miura, R., Relaño, M., Galbany, L., Sánchez-Blázquez, P., Pérez-Montero, E., Sánchez-Portal, M., Bongiovanni, A., Planelles, S., Quilis, V., Aubert, M., Guinet, D., Pomaréde, D., Weijmans, A. M., Raj, M. A., Aragón-Calvo, M. A., Azzaro, M., Bergond, G., Blazek, M., Cikota, S., Fernández-Martín, A., Gardini, A., Guijarro, A., Hermelo, I., Martín, P., Linares, J. I. Vico
Publikováno v:
A&A 689, A213 (2024)
We have learnt in the last decades that the majority of galaxies belong to high density regions interconnected in a sponge-like fashion. This large-scale structure is characterised by clusters, filaments, walls, where most galaxies concentrate, but a
Externí odkaz:
http://arxiv.org/abs/2405.04217
Autor:
Maria de Fátima Silva
Publikováno v:
Humanitas, Vol 67, Iss 0, Pp 253-255 (2015)
http://dx.doi.org/10.14195/2183-1718_67_20
Externí odkaz:
https://doaj.org/article/cb04cef30822467fa079d5e976b31968
Autor:
Kalinova, V., Colombo, D., Sánchez, S. F., Rosolowsky, E., Kodaira, K., García-Benito, R., Meidt, S. E., Davis, T. A., Romeo, A. B., Yu, S. -Y., Delgado, R. González, Lacerda, E. A. D.
Publikováno v:
A&A 665, A90 (2022)
It has been suggested that the gravitational potential can have a significant role in suppressing the star formation in the nearby galaxies. To establish observational constrains on this scenario, we investigate the connection between the dynamics, t
Externí odkaz:
http://arxiv.org/abs/2207.03872
Autor:
Kalinova, V., Colombo, D., Sánchez, S. F., Kodaira, K., García-Benito, R., Delgado, R. González, Rosolowsky, E., Lacerda, E. A. D.
Publikováno v:
A&A 648, A64 (2021)
The mechanisms that bring galaxies to strongly reduce their star formation activity (star-formation quenching) is still poorly understood. To better study galaxy evolution, we propose a classification based on the maps of the ionised hydrogen distrib
Externí odkaz:
http://arxiv.org/abs/2101.10019
Autor:
Silva, Maria de Fátima
Publikováno v:
Atlantís-review; Vol. 9 (2016)
http://dx.doi.org/10.14195/2183-1718_67_20
Autor:
Lyubenova, M., Martín-Navarro, I., van de Ven, G., Falcón-Barroso, J., Galbany, L., Gallazzi, A., García-Benito, R., Delgado, R. González, Husemann, B., La Barbera, F., Marino, R. A., Mast, D., Mendez-Abreu, J., Peletier, R. F. P., Sánchez-Blázquez, P., Sánchez, S. F., Trager, S. C., Bosch, R. C. E. van den, Vazdekis, A., Walcher, C. J., Zhu, L., Zibetti, S., Ziegler, B., Bland-Hawthorn, J., collaboration, the CALIFA
In this letter we describe how we use stellar dynamics information to constrain the shape of the stellar IMF in a sample of 27 early-type galaxies from the CALIFA survey. We obtain dynamical and stellar mass-to-light ratios, $\Upsilon_\mathrm{dyn}$ a
Externí odkaz:
http://arxiv.org/abs/1606.07448
Autor:
Sánchez, S. F., García-Benito, R., Zibetti, S., Walcher, C. J., Husemann, B., Mendoza, M. A., Galbany, L., Falcón-Barroso, J., Mast, D., Aceituno, J., Aguerri, J. A. L., Alves, J., Amorim, A. L., Ascasibar, Y., Barrado-Navascues, D., Barrera-Ballesteros, J., Bekeraitè, S., Bland-Hawthorn, J., Díaz, M. Cano, Fernandes, R. Cid, Cavichia, O., Cortijo, C., Dannerbauer, H., Demleitner, M., Díaz, A., Dettmar, R. J., de Lorenzo-Cáceres, A., del Olmo, A., Gallazzi, A., García-Lorenzo, B., de Paz, A. Gil, Delgado, R. González, Holmes, L., Iglésias-Páramo, J., Kehrig, C., Kelz, A., Kennicutt, R. C., Kleemann, B., Lacerda, E. A. D., Fernández, R. López, Sánchez, A. R. López, Lyubenova, M., Marino, R., Márquez, I., Mendez-Abreu, J., Mollá, M., Monreal-Ibero, A., Minakata, R. Ortega, Torres-Papaqui, J. P., Pérez, E., Rosales-Ortega, F. F., Roth, M. M., Sánchez-Blázquez, P., Schilling, U., Spekkens, K., Asari, N. Vale, Bosch, R. C. E. van den, van de Ven, G., Vilchez, J. M., Wild, V., Wisotzki, L., Yıldırım, A., Ziegler, B.
Publikováno v:
A&A 594, A36 (2016)
This paper describes the Third Public Data Release (DR3) of the Calar Alto Legacy Integral Field Area (CALIFA) survey. Science-grade quality data for 667 galaxies are made public, including the 200 galaxies of the Second Public Data Release (DR2). Da
Externí odkaz:
http://arxiv.org/abs/1604.02289
Autor:
Martin, M. Villar, Bellocchi, E., Stern, J., Almeida, C. Ramos, Tadhunter, C., Delgado, R. Gonzalez
We study the physical and kinematic properties of the narrow line region (NLR) of the nearest obscured quasar MRK 477 (z=0.037), using optical and near-infrared spectroscopy. We explore a diversity of aspects that provide a more complete understandin
Externí odkaz:
http://arxiv.org/abs/1509.01056
Autor:
Martín-Navarro, Ignacio, Vazdekis, Alexandre, La Barbera, Francesco, Falcón-Barroso, Jesús, Lyubenova, Mariya, van de Ven, Glenn, Ferreras, Ignacio, Sánchez, S. F., Trager, S. C., García-Benito, R., Mast, D., Mendoza, M. A., Sánchez-Blázquez, P., Delgado, R. González, Walcher, C. J., team, the CALIFA
Variations in the stellar initial mass function (IMF) have been invoked to explain the spectroscopic and dynamical properties of early-type galaxies. However, no observations have yet been able to disentangle the physical driver. We analyse here a sa
Externí odkaz:
http://arxiv.org/abs/1506.00638
Autor:
Sánchez, S. F., Vílchez, J. M., Walcher, C. J., Delgado, R González, de Paz, A Gil, Blázquez, P Sánchez, Marino, R, collaboration, The CALIFA
We present here a brief summary of the status of the on-going CALIFA survey with an em- phasis on the results that have been recently published. In particular, we make a summary of the most relevant results found regarding the properties of Hii regio
Externí odkaz:
http://arxiv.org/abs/1412.3153