Zobrazeno 1 - 10
of 13 866
pro vyhledávání: '"M Diaz"'
Autor:
C García, O Fernández, M Diaz, E Aurrecoechea, L Vega, F Elortza, M Azkargorta, E Ruiz, J Blanco, N Rivera, J Calvo, L Riancho, A De Diego-Sola, E Galindez, I Torre, E Cuende, A Intxaurbe, R Exposito, M Enjuanes, M Allande, I Iloro, M García-Vivar
Publikováno v:
Lupus Science and Medicine, Vol 9, Iss Suppl 2 (2022)
Externí odkaz:
https://doaj.org/article/d4efdc93eb27403a9546d99b7bf33a06
Autor:
AB Moreno-Castaño, A Ramos, M Pino, R Parra, C Altisent, F Vidal, I Corrales, N Borràs, S Torramadé-Moix, M Palomo, G Escolar, M Diaz-Ricart
Publikováno v:
Platelets, Vol 32, Iss 5, Pp 697-700 (2021)
Identification of qualitative variants of von Willebrand disease (VWD) can be a diagnostic challenge because of discrepant results obtained in the multiple laboratory tests available for its appropriate classification. We report two cases of infreque
Externí odkaz:
https://doaj.org/article/291079f0e4de447cab305789643ecaa6
Autor:
Vincentelli, F. M., Casella, P., Borghese, A., Cavecchi, Y., Mastroserio, G., Stella, L., Altamirano, D., Padilla, M. Armas, Baglio, M. C., Belloni, T. M., Casares, J., Cúneo, V. A., Degenaar, N., Trigo, M. Díaz, Fender, R., Maccarone, T., Malzac, J., Sánchez, D. Mata, Middleton, M., Migliari, S., Muñoz-Darias, T., O'Brien, K., Panizo-Espinar, G., Sánchez-Sierras, J., Russell, D. M., Uttley, P.
We report on the first simultaneous high-time resolution X-ray and infrared (IR) observations of a neutron star low mass X-ray binary in its hard state. We performed $\approx 2\,$h of simultaneous observations of 4U 1728-34 using HAWK-I@VLT, XMM-Newt
Externí odkaz:
http://arxiv.org/abs/2308.15570
Autor:
Eijnden, J. van den, Sidoli, L., Trigo, M. Diaz, Degenaar, N., Mellah, I. El, Fürst, F., Grinberg, V., Kretschmar, P., Martínez-Núñez, S., Miller-Jones, J. C. A., Postnov, K., Russell, T. D.
Neutron stars accreting from OB supergiants are often divided between persistently and transiently accreting systems, called Supergiant X-ray Binaries (SgXBs) and Supergiant Fast X-ray Transients (SFXTs). This dichotomy in accretion behaviour is typi
Externí odkaz:
http://arxiv.org/abs/2308.06021
Autor:
Gandhi, P., Kawamuro, T., Trigo, M. Díaz, Paice, J. A., Boorman, P. G., Cappi, M., Done, C., Fabian, A. C., Fukumura, K., Garcia, J. A., Greenwell, C. L., Guainazzi, M., Makishima, K., Tashiro, M. S., Tomaru, R., Tombesi, F., Ueda, Y.
Microcalorimeters have demonstrated success in delivering high spectral resolution, and have paved the path to revolutionary new science possibilities in the coming decade of X-ray astronomy. There are several research areas in compact object science
Externí odkaz:
http://arxiv.org/abs/2209.10576
Autor:
Saikia, Payaswini, Russell, David M., Baglio, M. C., Bramich, D. M., Casella, Piergiorgio, Trigo, M. Diaz, Gandhi, Poshak, Jiang, Jiachen, Maccarone, Thomas, Soria, Roberto, Noori, Hind Al, Yazeedi, Aisha Al, Alabarta, Kevin, Belloni, Tomaso, Bel, Marion Cadolle, Ceccobello, Chiara, Corbel, Stephane, Fender, Rob, Gallo, Elena, Homan, Jeroen, Koljonen, Karri, Lewis, Fraser, Markoff, Sera B., Miller-Jones, James C. A., Rodriguez, Jerome, Russell, Thomas D., Shahbaz, Tariq, Sivakoff, Gregory R., Testa, Vincenzo, Tetarenko, Alexandra J.
We present a detailed study of the evolution of the Galactic black hole transient GRS 1716-249 during its 2016-2017 outburst at optical (Las Cumbres Observatory), mid-infrared (Very Large Telescope), near-infrared (Rapid Eye Mount telescope), and ult
Externí odkaz:
http://arxiv.org/abs/2205.04452
Autor:
Segura, N. Castro, Knigge, C., Long, K. S., Altamirano, D., Padilla, M. Armas, Bailyn, C., Buckley, D. A. H., Buisson, D. J. K., Casares, J., Charles, P., Combi, J. A., Cúneo, V. A., Degenaar, N. D., del Palacio, S., Trigo, M. Díaz, Fender, R., Gandhi, P., Georganti, M., Gutiérrez, C., Santisteban, J. V. Hernandez, Jiménez-Ibarra, F., Matthews, J., Méndez, M., Middleton, M., Muñoz-Darias, T., Arabacı, M. Özbey, Pahari, M., Rhodes, L., Russell, T. D., Scaringi, S., Eijnden, J. van den, Vasilopoulos, G., Vincentelli, F. M., Wiseman, P.
All disc-accreting astrophysical objects produce powerful outflows. In binaries containing neutron stars (NS) or black holes, accretion often takes place during violent outbursts. The main disc wind signatures during these eruptions are blue-shifted
Externí odkaz:
http://arxiv.org/abs/2203.01372
Publikováno v:
In Computers and Electrical Engineering December 2024 120 Part B
Autor:
S ORTOLANI, M DIAZ-CURIEL
Publikováno v:
Остеопороз и остеопатии, Vol 10, Iss 2 (2007)
Externí odkaz:
https://doaj.org/article/99dbb8b2cb764eefbb09c7c400899304
Autor:
Russell, T. D., Degenaar, N., Eijnden, J. van den, Del Santo, M., Segreto, A., Altamirano, D., Beri, A., Trigo, M. Diaz, Miller-Jones, J. C. A.
The persistently bright ultra-compact neutron star low-mass X-ray binary 4U 1820$-$30 displays a $\sim$170 d accretion cycle, evolving between phases of high and low X-ray modes, where the 3 -- 10 keV X-ray flux changes by a factor of up to $\approx
Externí odkaz:
http://arxiv.org/abs/2107.12491