Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Rodríguez Castillo, G A"'
Autor:
D'Aì, A., Pinto, C., Del Santo, M., Pintore, F., Soria, R., Robba, A., Ambrosi, E., Alston, W., Barret, D., Fabian, A. C., Fürst, F., Kara, E., Kosec, P., Middleton, M., Roberts, T., Rodriguez-Castillo, G., Walton, D. J.
Soft Ultra-Luminous X-ray (ULXs) sources are a subclass of the ULXs that can switch from a supersoft spectral state, where most of the luminosity is emitted below 1 keV, to a soft spectral state with significant emission above 1 keV. In a few systems
Externí odkaz:
http://arxiv.org/abs/2108.09221
Autor:
De Luca, A., Salvaterra, R., Belfiore, A., Carpano, S., D'Agostino, D., Haberl, F., Israel, G. L., Law-Green, D., Lisini, G., Marelli, M., Novara, G., Read, A. M., Rodriguez-Castillo, G., Rosen, S. R., Salvetti, D., Tiengo, A., Vianello, G., Watson, M. G., Delvaux, C., Dickens, T., Esposito, P., Greiner, J., Haemmerle, H., Kreikenbohm, A., Kreykenbohm, S., Oertel, M., Pizzocaro, D., Pye, J. P., Sandrelli, S., Stelzer, B., Wilms, J., Zagaria, F.
Temporal variability in flux and spectral shape is ubiquitous in the X-ray sky and carries crucial information about the nature and emission physics of the sources. The EPIC instrument on board the XMM-Newton observatory is the most powerful tool for
Externí odkaz:
http://arxiv.org/abs/2105.02895
Autor:
Pintore, Fabio, Motta, S., Pinto, C., Bernardini, M. G., Rodriguez-Castillo, G., Salvaterra, R., Israel, G. L., Esposito, P., Ambrosi, E., Salvaggio, C., Zampieri, L., Wolter, A.
Ultraluminous X-ray sources are considered amongst the most extremely accreting objects in the local Universe. The recent discoveries of pulsating neutron stars in ULXs strengthened the scenario of highly super-Eddington accretion mechanisms on stell
Externí odkaz:
http://arxiv.org/abs/2103.14541
Autor:
Marchesini, E. J., Masetti, N., Chavushyan, V., Cellone, S. A., Andruchow, I., Bassani, L., Bazzano, A., Jiménez-Bailón, E., Landi, R., Malizia, A., Palazzi, E., Patiño-Álvarez, V., Rodríguez-Castillo, G. A., Stephen, J. B., Ubertini, P.
Publikováno v:
A&A 596, A10 (2016)
Context. Based on their overwhelming dominance among associated Fermi gamma ray catalogue sources, it is expected that a large fraction of the unidentified Fermi objects are blazars. Through crossmatching between the positions of unidentified gamma r
Externí odkaz:
http://arxiv.org/abs/1608.05429
Autor:
Fürst, F., Walton, D. J., Israel, G. L., Bachetti, M., Barret, D., Brightman, M., Earnshaw, H. P., Fabian, A. C., Heida, M., Imbrogno, M., Middleton, M. J., Pinto, C., Salvaterra, R., Roberts, T. P., Rodríguez Castillo, G. A., Webb, N. A.
NGC 5907 ULX1 is the most luminous ultra-luminous X-ray pulsar (ULXP) known to date, reaching luminosities in excess of 1e41 erg/s. The pulsar is known for its fast spin-up during the on-state. Here, we present a long-term monitoring of the X-ray flu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::35f3a8ccd97bc248d11ef31d6b456901
https://eprints.soton.ac.uk/477446/
https://eprints.soton.ac.uk/477446/
Autor:
Imbrogno, M, Israel, G L, Rodríguez Castillo, G A, Buckley, D A H, Coti Zelati, F, Rea, N, Monageng, I M, Casella, P, Stella, L, Haberl, F, Esposito, P, Tombesi, F, De Luca, A, Tiengo, A
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Oct2023, Vol. 524 Issue 4, p5566-5574, 9p
Autor:
Cellone, S. A., Andruchow, I., Marchesini, E. J., Rodríguez-Castillo, G. A., Masetti, N., Chavushyan, V., Patiño-Álvarez, V., Bassani, L., Landi, R., Malizia, A., Palazzi, E., Stephen, J. B., Bazzano, A., Ubertini, P., Jiménez-Bailón, E.
Publikováno v:
Astronomy & Astrophysics / Astronomie et Astrophysique; Dec2016, Vol. 596, p1-9, 9p, 2 Charts, 2 Graphs
Publikováno v:
Monthly Notices of the Royal Astronomical Society; 11/11/2016, Vol. 462 Issue 4, p4371-4385, 15p, 2 Charts, 5 Graphs