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Autor Mirabal Barrios, Néstor |
Documentos disponibles escritos por este autor (4)
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Antoranz Canales, Pedro ; Barrio Uña, Juan Abel ; Bernardino Santos, Teodoro ; Contreras González, José Luis ; Hassan, Tarek ; Mirabal Barrios, Néstor ; Miranda Pantoja, José Miguel ; Tejedor Álvarez, Luis Ángel ; Vegas Azcárate, Ignacio | Springer | 2011-12Ground-based gamma-ray astronomy has had a major breakthrough with the impressive results obtained using systems of imaging atmospheric Cherenkov telescopes. Ground-based gamma-ray astronomy has a huge potential in astrophysics, particle physics[...]texto impreso
Antoranz Canales, Pedro ; Barrio Uña, Juan Abel ; Bernardino Santos, Teodoro ; Contreras González, José Luis ; Fonseca González, Mª Victoria ; Hassan, Tarek ; López Moya, Marcos ; Mirabal Barrios, Néstor ; Miranda Pantoja, José Miguel ; Satalecka, Konstanzja ; Scapin, Valeria ; Tejedor Álvarez, Luis Ángel ; Yebras Rivera, José Manuel | Elsevier Science BV | 2013-03The Cherenkov Telescope Array (CTA) is a new observatory for very high-energy (VHE) gamma rays. CTA has ambitions science goals, for which it is necessary to achieve full-sky coverage, to improve the sensitivity by about an order of magnitude, t[...]texto impreso
Arqueros Martínez, Fernando ; Barrio Uña, Juan Abel ; Contreras González, José Luis ; Franco Peláez, Francisco Javier ; López Moya, Marcos ; Mirabal Barrios, Néstor ; Nievas Rosillo, Mireia ; Rosado Vélez, Jaime ; Tejedor Álvarez, Luis Ángel | American Astronomical Society | 2017-05-10We perform simulations for future Cherenkov Telescope Array (CTA) observations of RX J1713.7?3946, a young supernova remnant (SNR) and one of the brightest sources ever discovered in very high energy (VHE) gamma rays. Special attention is paid t[...]texto impreso
Nichols, Matthew ; Mirabal Barrios, Néstor ; Agertz, Oscar ; Lockman, Felix J. ; Bland-Hawthorn, Joss | Oxford Univ Press | 2014-08-21Under conservative assumptions about the Galaxy, the derived velocity of the Smith Cloud indicates that it will have undergone at least one passage of the Galactic disc. Using hydrodynamic simulations, we examine the present-day structure of the[...]