Zobrazeno 1 - 10
of 43
pro vyhledávání: '"Florido, Estrella"'
Autor:
Conrado, Ana M., Delgado, Rosa M. González, García-Benito, Rubén, Pérez, Isabel, Verley, Simon, Ruiz-Lara, Tomás, Sánchez-Menguiano, Laura, Puertas, Salvador Duarte, Jiménez, Andoni, Domínguez-Gómez, Jesús, Espada, Daniel, Argudo-Fernández, María, Alcázar-Laynez, Manuel, Blázquez-Calero, Guillermo, Bidaran, Bahar, Zurita, Almudena, Peletier, Reynier, Torres-Ríos, Gloria, Florido, Estrella, Martínez, Mónica Rodríguez, del Moral-Castro, Ignacio, van de Weygaert, Rien, Falcón-Barroso, Jesús, Lugo-Aranda, Alejandra Z., Sánchez, Sebastián F., van der Hulst, Thijs, Courtois, Hélène M., Ferré-Mateu, Anna, Sánchez-Blázquez, Patricia, Román, Javier, Aceituno, Jesús
Publikováno v:
A&A 687, A98 (2024)
The Universe is shaped as a web-like structure, formed by clusters, filaments, and walls that leave large volumes in between named voids. Galaxies in voids have been found to be of a later type, bluer, less massive, and to have a slower evolution tha
Externí odkaz:
http://arxiv.org/abs/2404.10823
Autor:
Domínguez-Gómez, Jesús, Pérez, Isabel, Ruiz-Lara, Tomás, Peletier, Reynier F., Sánchez-Blázquez, Patricia, Lisenfeld, Ute, Bidaran, Bahar, Falcón-Barroso, Jesús, Alcázar-Laynez, Manuel, Argudo-Fernández, María, Blázquez-Calero, Guillermo, Courtois, Hélène, Puertas, Salvador Duarte, Espada, Daniel, Florido, Estrella, García-Benito, Rubén, Jiménez, Andoni, Kreckel, Kathryn, Relaño, Mónica, Sánchez-Menguiano, Laura, van der Hulst, Thijs, van de Weygaert, Rien, Verley, Simon, Zurita, Almudena
Publikováno v:
A&A 680, A111 (2023)
Void galaxies are essential for understanding the physical processes that drive galaxy evolution because they are less affected by external factors than galaxies in denser environments, that is, in filaments, walls, and clusters. The stellar metallic
Externí odkaz:
http://arxiv.org/abs/2310.11412
Autor:
Pérez-Montero, Enrique, Zinchenko, Igor, Vílchez, José M., Zurita, Almudena, Florido, Estrella, Pérez-Díaz, Borja
Publikováno v:
A&A 669, A88 (2023)
We explore the so-called softness diagram -- whose main function is to provide the hardness of the ionizing radiation in star-forming regions -- in order to check whether hot and old low-mass evolved stars (HOLMES) are significant contributors to the
Externí odkaz:
http://arxiv.org/abs/2212.03216
We use a sample of 536 \hii\ regions located in nearby spirals, with an homogeneous determination of their $T_e$-based abundances, to obtain new empirical calibrations of the N2O2, N2S2, O3N2, and N2 strong-line indices to estimate the nitrogen-to-ox
Externí odkaz:
http://arxiv.org/abs/2203.17021
Autor:
Blázquez-Calero, Guillermo, Florido, Estrella, Pérez, Isabel, Zurita, Almudena, Grand, Robert J. J., Fragkoudi, Francesca, Gómez, Facundo A., Marinacci, Federico, Pakmor, Rüdiger
In this work we analyse the structural and photometric properties of 21 barred simulated galaxies from the Auriga Project. These consist of Milky Way-mass magneto-hydrodynamical simulations in a $\Lambda$CDM cosmological context. In order to compare
Externí odkaz:
http://arxiv.org/abs/1911.01964
Autor:
Kalinova, Veselina, Colombo, Dario, Rosolowsky, Erik, Kannan, Rahul, Galbany, Lluís, García-Benito, Rubén, Delgado, Rosa González, Sánchez, Sebastian F., Ruiz-Lara, Tomás, Méndez-Abreu, Jairo, Catalán-Torrecilla, Cristina, Sánchez-Menguiano, Laura, de Lorenzo-Cáceres, Adriana, Costantin, Luca, Florido, Estrella, Kodaira, Keiichi, Marino, Raffaella A., Läsker, Ronald, Bland-Hawthorn, Joss
Publikováno v:
Mon. Not. R. Astron. Soc. (2017) 469 (3): 2539-2594
We present a galaxy classification system for 238 (E1-Sdm) CALIFA (Calar Alto Legacy Integral Field Area) galaxies based on the shapes and amplitudes of their circular velocity curves (CVCs). We infer the CVCs from the de-projected surface brightness
Externí odkaz:
http://arxiv.org/abs/1509.03352
Autor:
Wild, Vivienne, Rosales-Ortega, Fabian, Falcon-Barroso, Jesus, Garcia-Benito, Ruben, Gallazzi, Anna, Delgado, Rosa M. Gonzalez, Bekeraite, Simona, Pasquali, Anna, Johansson, Peter H., Lorenzo, Begona Garcia, van de Ven, Glenn, Pawlik, Milena, Perez, Enrique, Monreal-Ibero, Ana, Lyubenova, Mariya, Fernandes, Roberto Cid, Mendez-Abreu, Jairo, Barrera-Ballesteros, Jorge, Kehrig, Carolina, Iglesias-Paramo, Jorge, Bomans, Dominik J., Marquez, Isabel, Johnson, Benjamin D., Kennicutt, Robert C., Husemann, Bernd, Mast, Damian, Sanchez, Sebastian F., Walcher, C. Jakob, Alves, Joao, Aguerri, Alfonso L., Herrero, Almudena Alonso, Bland-Hawthorn, Joss, Catalan-Torrecilla, Cristina, Florido, Estrella, Gomes, Jean Michel, Jahnke, Knud, Lopez-Sanchez, A. R., de Lorenzo-Caceres, Adriana, Marino, Raffaella A., Marmol-Queralto, Esther, Olden, Patrick, del Olmo, Ascension, Papaderos, Polychronis, Quirrenbach, Andreas, Vilchez, Jose M., Ziegler, Bodo
Publikováno v:
A&A 567, A132 (2014)
We present optical integral field spectroscopy (IFS) observations of the Mice, a major merger between two massive (>10^11Msol) gas-rich spirals NGC4676A and B, observed between first passage and final coalescence. The spectra provide stellar and gas
Externí odkaz:
http://arxiv.org/abs/1405.7814
Akademický článek
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Autor:
Battaner, Eduardo, Florido, Estrella
Following the model of magnetically supported rotation of spiral galaxies, the inner disk rotation is dominated by gravity but magnetism is not negligible at radii where the rotation curve becomes flat, and indeed becomes dominant at very large radii
Externí odkaz:
http://arxiv.org/abs/astro-ph/0503657
Poster presented at the conference 'Galactic bars: driving and decoding galaxy evolution', celebrated in Granada (Spain), 3 - 7July, 2023
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3af3ace04ed4ed9894b6fa5100c05588