Zobrazeno 1 - 10
of 1 422
pro vyhledávání: '"Nobili, L."'
Autor:
Chiarello, D., Cognolato, E., Francione, S., Nobile, G., Bosisio, L., Barbagallo, G., Pacetti, M., Tortora, D., Cantalupo, G., Nobili, L., Consales, A.
Publikováno v:
In Epilepsy & Behavior April 2024 153
Publikováno v:
In NeuroImage 15 May 2023 272
Autor:
Miano, S., Fanfulla, F., Nobili, L., Heinzer, R., Haba-Rubio, J., Berger, M., Cereda, C.W., Schmidt, M.H., Manconi, M., Bassetti, C.L.A.
Publikováno v:
In Sleep Medicine October 2022 98:106-113
Autor:
Russo, S., Pigorini, A., Mikulan, E., Sarasso, S., Rubino, A., Zauli, F.M., Parmigiani, S., d'Orio, P., Cattani, A., Francione, S., Tassi, L., Bassetti, C.L.A., Lo Russo, G., Nobili, L., Sartori, I., Massimini, M.
Publikováno v:
In NeuroImage 1 July 2021 234
Autor:
Bernasconi, C., Ott, S.R., Fanfulla, F., Miano, S., Horvath, T., Seiler, A., Cereda, C.W., Brill, A.-K., Young, P., Nobili, L., Manconi, M., Bassetti, C.L.A.
Publikováno v:
In Sleep Medicine: X December 2020 2
Autor:
Turolla, R., Nobili, L.
The problem of computing the pulse profiles from thermally emitting spots on the surface of a neutron star in general relativity is reconsidered. We show that it is possible to extend Beloborodov (2002) approach to include (multiple) spots of finite
Externí odkaz:
http://arxiv.org/abs/1303.6835
Autor:
Panzeri, G., Muller, D., Accogli, A., Gibertini, E., Mauri, E., Rossi, F., Nobili, L., Magagnin, L.
Publikováno v:
In Electrochimica Acta 10 February 2019 296:465-472
We present the first detailed joint modelling of both the timing and spectral properties during the outburst decay of transient anomalous X-ray pulsars. We consider the two sources XTE J1810-197 and CXOU J164710.2-455216, and describe the source decl
Externí odkaz:
http://arxiv.org/abs/1103.0955
Anomalous X-ray pulsars (AXPs) and soft gamma repeaters (SGRs) are two small classes of X-ray sources strongly suspected to host a magnetar, i.e. an ultra-magnetized neutron star with $B\approx 10^14-10^15 G. Many SGRs/AXPs are known to be variable,
Externí odkaz:
http://arxiv.org/abs/1007.5466
Within the magnetar scenario, the "twisted magnetosphere" model appears very promising in explaining the persistent X-ray emission from the Soft Gamma Repeaters and the Anomalous X-ray Pulsars (SGRs and AXPs). In the first two papers of the series, w
Externí odkaz:
http://arxiv.org/abs/0906.1135