Zobrazeno 1 - 10
of 96
pro vyhledávání: '"Sánchez-Menguiano, L."'
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
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:
Domínguez-Gómez, J., Pérez, I., Ruiz-Lara, T., Peletier, R. F., Sánchez-Blázquez, P., Lisenfeld, U., Falcón-Barroso, J., Alcázar-Laynez, M., Argudo-Fernández, M., Blázquez-Calero, G., Courtois, H., Puertas, S. Duarte, Espada, D., Florido, E., García-Benito, R., Jiménez, A., Kreckel, K., Relaño, M., Sánchez-Menguiano, L., van der Hulst, T., van de Weygaert, R., Verley, S., Zurita, A.
Galaxies in the Universe are distributed in a web-like structure characterised by different large-scale environments: dense clusters, elongated filaments, sheetlike walls, and under-dense regions, called voids. The low density in voids is expected to
Externí odkaz:
http://arxiv.org/abs/2306.16818
Autor:
Lugo-Aranda, A. Z., Sánchez, S. F., Espinosa-Ponce, C., López-Cobá, C., Galbany, L., Barrera-Ballesteros, J. K., Sánchez-Menguiano, L., Anderson, J. P.
We present a new code named pyHIIextractor, which detects and extracts the main features (positions and radii) of clumpy ionized regions, i.e. candidate HII regions, using H{\alpha} emission line images. Our code is optimized to be used on the datapr
Externí odkaz:
http://arxiv.org/abs/2204.04252
Autor:
Rousseau-Nepton, L., Martin, R. P., Robert, C., Drissen, L., Amram, P., Prunet, S., Martin, T., Moumen, I., Adamo, A., Alarie, A., Barmby, P., Boselli, A., Bresolin, F., Bureau, M., Chemin, L., Fernandes, R. C., Combes, F., Crowder, C., Della Bruna, L., Egusa, F., Epinat, B., Ksoll, V. F., Girard, M., Llanos, V. Gómez, Gouliermis, D., Grasha, K., Higgs, C., Hlavacek-Larrondo, J., Ho, I. -T., Iglesias-Páramo, J., Joncas, G., Kam, Z. S., Karera, P., Kennicutt, R. C., Klessen, R. S., Lianou, S., Liu, L., Liu, Q., de Amorim, A. Luiz, Lyman, J. D., Martel, H., Mazzilli-Ciraulo, B., McLeod, A. F., Melchior, A-L., Millan, I., Mollá, M., Momose, R., Morisset, C., Pan, H. -A., Pati, A. K., Pellerin, A., Pellegrini, E., Pérez, I., Petric, A., Plana, H., Rahner, D., Lara, T. Ruiz, Sánchez-Menguiano, L., Spekkens, K., Stasińska, G., Takamiya, M., Asari, N. Vale, Vílchez, J. M.
SIGNALS, the Star formation, Ionized Gas, and Nebular Abundances Legacy Survey, is a large observing program designed to investigate massive star formation and HII regions in a sample of local extended galaxies. The program will use the imaging Fouri
Externí odkaz:
http://arxiv.org/abs/1908.09017
The fundamental metallicity relation (FMR) states that galaxies of the same stellar mass but larger star formation rate (SFR) tend to have smaller gas-phase metallicity (). It is thought to be fundamental because it naturally arises from the stoc
Externí odkaz:
http://arxiv.org/abs/1905.05826
Autor:
Lopez-Coba, C., Sanchez, S. F., Cruz-Gonzalez, I., Binette, L., Galbany, L., Kruhler, T., Rodrıguez, L. F., Barrera-Ballesteros, J. K., Sanchez-Menguiano, L., Walcher, C. J., Aquino-Ortız, E., Anderson, J. P.
We report the detection of a highly collimated linear emission-line structure in the spiral galaxy NGC\,232 through the use of integral field spectroscopy data from the All-weather MUse Supernova Integral field Nearby Galaxies (AMUSING) survey. This
Externí odkaz:
http://arxiv.org/abs/1711.02785
Autor:
Mendez-Abreu, J., Aguerri, J. A. L., Falcon-Barroso, J., Ruiz-Lara, T., Sanchez-Menguiano, L., de Lorenzo-Caceres, A., Costantin, L., Catalan-Torrecilla, C., Zhu, L., Sanchez-Blazquez, P., Florido, E., Corsini, E. M., Wild, V., Lyubenova, M., van de Ven, G., Sanchez, S. F., Bland-Hawthorn, J., Galbany, L., Garcia-Benito, R., Garcia-Lorenzo, B., Delgado, R. M. Gonzalez, Lopez-Sanchez, A. R., Marino, R. A., Marquez, I., Ziegler, B.
We study a sample of 28 S0 galaxies extracted from the integral-field spectroscopic (IFS) survey CALIFA. We combine an accurate two-dimensional (2D) multi-component photometric decomposition with the IFS kinematic properties of their bulges to unders
Externí odkaz:
http://arxiv.org/abs/1710.09349
Autor:
Sánchez-Menguiano, L., Sánchez, S. F., Pérez, I., Ruiz-Lara, T., Galbany, L., Anderson, J. P., Krühler, T., Kuncarayakti, H., Lyman, J. D.
Publikováno v:
A&A 609, A119 (2018)
We characterise the oxygen abundance radial distribution of a sample of 102 spiral galaxies observed with VLT/MUSE using the O3N2 calibrator. The high spatial resolution of the data allows us to detect 14345 HII regions with the same image quality as
Externí odkaz:
http://arxiv.org/abs/1710.01188
Autor:
Catalán-Torrecilla, C., de Paz, A. Gil, Castillo-Morales, A., Méndez-Abreu, J., Falcón-Barroso, J., Bekeraite, S., Costantin, L., de Lorenzo-Cáceres, A., Florido, E., García-Benito, R., Husemann, B., Iglesias-Páramo, J., Kennicutt, R. C., Mast, D., Pascual, S., Ruiz-Lara, T., Sánchez-Menguiano, L., Sánchez, S. F., Walcher, C. J., Bland-Hawthorn, J., Puertas, S. Duarte, Marino, R. A., Masegosa, J., Sánchez-Blázquez, P., Collaboration, CALIFA
We estimate the current extinction-corrected H$\alpha$ star formation rate (SFR) of the different morphological components that shape galaxies (bulges, bars, and disks). We use a multi-component photometric decomposition based on SDSS imaging to CALI
Externí odkaz:
http://arxiv.org/abs/1709.01035
Autor:
Sánchez-Menguiano, L., Sánchez, S. F., Pérez, I., Debattista, V. P., Ruiz-Lara, T., Florido, E., Cavichia, O., Galbany, L., Marino, R. A., Mast, D., Sánchez-Blázquez, P., Méndez-Abreu, J., de Lorenzo-Cáceres, A., Catalán-Torrecilla, C., Cano-Díaz, M., Márquez, I., McIntosh, D. H., Ascasibar, Y., García-Benito, R., Delgado, R. M. Gónzalez, Kehrig, C., López-Sánchez, Á. R., Mollá, M., Bland-Hawthorn, J., Walcher, C. J., Costantin, L.
Publikováno v:
A&A 603, A113 (2017)
Spiral arms are the most singular features in disc galaxies. These structures can exhibit different patterns, namely grand design and flocculent arms, with easily distinguishable characteristics. However, their origin and the mechanisms shaping them
Externí odkaz:
http://arxiv.org/abs/1705.05733