Zobrazeno 1 - 10
of 10 520
pro vyhledávání: '"LÓPEZ, A. E."'
Autor:
Esparza-Arredondo, D., Almeida, C. Ramos, Audibert, A., Pereira-Santaella, M., García-Bernete, I., García-Burillo, S., Shimizu, T., Davies, R., Muñoz, L. Hermosa, Alonso-Herrero, A., Combes, F., Speranza, G., Zhang, L., Campbell, S., Bellocchi, E., Bunker, A. J., Díaz-Santos, T., García-Lorenzo, B., González-Martín, O., Hicks, E. K. S., Labiano, A., Levenson, N. A., Ricci, C., Rosario, D., Hoenig, S., Packham, C., Stalevski, M., Fuller, L., Izumi, T., López-Rodríguez, E., Rigopoulou, D., Rouan, D., Ward, M.
Understanding the processes that drive the morphology and kinematics of molecular gas in galaxies is crucial for comprehending star formation and, ultimately, galaxy evolution. Using data obtained with the James Webb Space Telescope (JWST) and the At
Externí odkaz:
http://arxiv.org/abs/2411.12398
Autor:
Kuchera, A. N., Ryan, G., Selby, G., Snider, D., Anderson, S., Almaraz-Calderon, S., Baby, L. T., Brown, B. A., Hanselman, K., Lopez-Saavedra, E., Macon, K. T., McCann, G. W., Kemper, K. W., Spieker, M., Wiedenhöver, I.
The resonance region of $^{11}$B covering excitation energies from 8.4 MeV to 13.6 MeV was investigated with the $(d,p)$ reaction performed on an enriched $^{10}$B target at the Florida State University Super-Enge Split-Pole Spectrograph of the John
Externí odkaz:
http://arxiv.org/abs/2411.09831
The active galactic nucleus (AGN) within M87, a giant elliptical galaxy, is responsible for one of the closest kiloparsec-scale relativistic jet to Earth. We unearthed unpublished M87 polarization maps taken with the Faint Object Camera (FOC) aboard
Externí odkaz:
http://arxiv.org/abs/2410.07903
Autor:
Sengupta, D., Torres-Albà, N., Pizzetti, A., López, I. E., Marchesi, S., Vignali, C., Barchiesi, L., Cox, I., Gaspari, M., Zhao, X., Ajello, M., Esposito, F.
Most of the super-massive black holes in the Universe accrete material in an obscured phase. While it is commonly accepted that the "dusty torus" is responsible for the nuclear obscuration, its geometrical, physical, and chemical properties are far f
Externí odkaz:
http://arxiv.org/abs/2410.02878
Autor:
López-López, X., Bolzonella, M., Pozzetti, L., Salvato, M., Bisigello, L., Feltre, A., López, I. E., Viitanen, A., Allevato, V., Bongiorno, A., Girelli, G., Buchner, J., Charlot, S., Ricci, F., Schreiber, C., Zamorani, G.
Publikováno v:
A&A 691, A136 (2024)
Aims. We present MAMBO, a flexible and efficient workflow to build empirical galaxy and Active Galactic Nuclei (AGN) mock catalogues that reproduce the physical and observational properties of these sources. Methods. We start from simulated dark matt
Externí odkaz:
http://arxiv.org/abs/2409.06700
Autor:
García-Bernete, I., Rigopoulou, D., Donnan, F. R., Alonso-Herrero, A., Pereira-Santella, M., Shimizu, T., Davies, R., Roche, P. F., García-Burillo, S., Labiano, A., Muñoz, L. Hermosa, Zhang, L., Audibert, A., Bellocchi, E., Bunker, A., Combes, F., Delaney, D., Esparza-Arredondo, D., Gandhi, P., González-Martín, O., Hönig, S. F., Imanishi, M., Hicks, E. K. S., Fuller, L., Leist, M., Levenson, N. A., Lopez-Rodriguez, E., Packham, C., Almeida, C. Ramos, Ricci, C., Stalevski, M., Martín, M. Villar, Ward, M. J.
Publikováno v:
A&A 691, A162 (2024)
We analyze JWST MIRI/MRS observations of the infrared PAH bands in the nuclear and circumnuclear regions of local AGN from the GATOS Survey. In this work, we examine the PAH properties in the circumnuclear regions of AGN and AGN-outflows, and compare
Externí odkaz:
http://arxiv.org/abs/2409.05686
Autor:
Tavera-Vázquez, Antonio, Montalvan-Sorrosa, Danai, Perez-Lemus, Gustavo, Rodriguez-Lopez, Otilio E., Martinez-Gonzalez, Jose A., Manoharan, Vinothan N., de Pablo, Juan J.
Motile liquid crystal (LC) colloids show peculiar behavior due to the high sensitivity to external stimuli driven by the LC elastic and surface effects. However, few studies focus on harnessing the LC phase transitions to propel colloidal inclusions
Externí odkaz:
http://arxiv.org/abs/2409.04912
Autor:
Zhao, Xiurui, Marchesi, Stefano, Ajello, Marco, Civano, Francesca, Gilli, Roberto, Lanzuisi, Giorgio, López, Iván E., Silver, Ross, Torres-Albà, Nuria, Boorman, Peter G., Pizzetti, Andrealuna
We present a comprehensive X-ray analysis and spectral energy distribution (SED) fitting of WISEA J171419.96+602724.6, an extremely luminous type 2 quasar at $z$ = 2.99. The source was suggested as a candidate Compton-thick (column density N$_{\rm H}
Externí odkaz:
http://arxiv.org/abs/2409.01960
Autor:
Bertola, E., Circosta, C., Ginolfi, M., Mainieri, V., Vignali, C., Rivera, G. Calistro, Ward, S. R., Lopez, I. E., Pensabene, A., Alexander, D. M., Bischetti, M., Brusa, M., Cappi, M., Comastri, A., Contursi, A., Cicone, C., Cresci, G., Dadina, M., D'Amato, Q., Feltre, A., Harrison, C. M., Kakkad, D., Lamperti, I., Lanzuisi, G., Mannucci, F., Marconi, A., Perna, M., Piconcelli, E., Puglisi, A., Ricci, F., Scholtz, J., Tozzi, G., Vietri, G., Zamorani, G., Zappacosta, L.
The energy released by AGN has the potential to heat or remove the gas of the ISM, thus likely impacting the cold molecular gas reservoir of host galaxies at first, with star formation following on longer timescales. Previous works on high-z galaxies
Externí odkaz:
http://arxiv.org/abs/2408.16821
Autor:
Mazzolari, Giovanni, Scholtz, Jan, Maiolino, Roberto, Gilli, Roberto, Traina, Alberto, López, Ivan E., Übler, Hannah, Trefoloni, Bartolomeo, D'Eugenio, Francesco, Ji, Xihan, Mignoli, Marco, Vito, Fabio, Brusa, Marcella
In this work, we spectroscopically select narrow-line AGN (NLAGN) among the $\sim 300$ publicly available medium-resolution spectra of the CEERS Survey. Using both traditional and newly identified emission line NLAGN diagnostics diagrams, we identifi
Externí odkaz:
http://arxiv.org/abs/2408.15615