835 citations
- National Interuniversity Consortium for the Physical Sciences of MatterIT34 papers
- Osservatorio Astronomico di PalermoIT25 papers
- National Institute for AstrophysicsIT12 papers
- Astronomical Observatory of RomeIT11 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di CagliariIT11 papers
- University of CagliariIT11 papers
- University of Rome Tor VergataIT9 papers
- Santa Fe InstituteUS7 papers
- Arcetri Astrophysical ObservatoryIT5 papers
- Edison (Italy)IT5 papers
- Centre National de la Recherche ScientifiqueFR4 papers
- European Space Research and Technology CentreNL4 papers
5 papers · 1 filter
Simbol-X capability of detecting the non-thermal emission of stellar flares
C. Argiroffi, G. Micela, A. Maggio
We investigate the capability of detecting, with Simbol-X, non-thermal emission during stellar flares, and distinguishing it from hot thermal emission. We find that flare non-therm…
Detection of the Cherenkov light diffused by Sea Water with the ULTRA Experiment
G. Agnetta, P. Assis, B. Biondo +26
The study of Ultra High Energy Cosmic Rays represents one of the most challenging topic in the Cosmic Rays and in the Astroparticle Physics fields. The interaction of primary parti…
Shock oscillation model for QPOs in stellar-mass and supermassive black holes
T. Okuda, V. Teresi, D. Molteni
We numerically examine centrifugally supported shock waves in 2D rotating accretion flows around a stellar-mass (10M_sun) and a supermassive (10^6M_sun) black holes over a wide ran…
High Resolution X-ray Spectroscopy of Pre-Main-Sequence Stars: TWA 5 and PZ Tel
C. Argiroffi, J. J. Drake, F. R. Harnden +5
We report on the analysis of high resolution X-ray spectra of two pre-main-sequence stars: TWA 5 (observed with XMM-Newton) and PZ Telescopii (observed with Chandra/HETGS). TWA 5 i…
To accrete or not to accrete: the dilemma of the recycling scenario
L. Burderi, F. D'Antona, T. Di Salvo +3
We study the evolution of a low-mass X-ray binary by coupling a binary stellar evolution code with a general relativistic code that describes the behaviour of the neutron star. We…