Zobrazeno 1 - 10
of 303
pro vyhledávání: '"RAPISARDA, S."'
Autor:
Albayati, A. C., Altamirano, D., Jaisawal, G. K., Bult, P., Rapisarda, S., Mancuso, G. C., Güver, T., Arzoumanian, Z., Chakrabarty, D., Chenevez, J., Court, J. M. C., Gendreau, K. C., Guillot, S., Keek, L., Malacaria, C., Strohmayer, T. E.
Publikováno v:
MNRAS, 501 (2021) 261-268
MAXI J1807+132 is a low-mass X-ray binary (LMXB) first detected in outburst in 2017. Observations during the 2017 outburst did not allow for an unambiguous identification of the nature of the compact object. MAXI J1807+132 was detected in outburst ag
Externí odkaz:
http://arxiv.org/abs/2011.10448
Autor:
Russell, T. D., Tetarenko, A. J., Miller-Jones, J. C. A., Sivakoff, G. R., Parikh, A. S., Rapisarda, S., Wijnands, R., Corbel, S., Tremou, E., Altamirano, D., Baglio, M. C., Ceccobello, C., Degenaar, N., Eijnden, J. van den, Fender, R., Heywood, I., Krimm, H. A., Lucchini, M., Markoff, S., Russell, D. M., Soria, R., Woudt, P. A.
MAXI J1535-571 is a Galactic black hole candidate X-ray binary that was discovered going into outburst in 2017 September. In this paper, we present comprehensive radio monitoring of this system using the Australia Telescope Compact Array (ATCA), as w
Externí odkaz:
http://arxiv.org/abs/1906.00998
We present a timing analysis of threeRossi X-ray Timing Explorer observations of the black hole binary Cygnus X-1 with the propagating mass accretion rate fluctuations model PROPFLUC. The model simultaneously predicts power spectra, time lags, and co
Externí odkaz:
http://arxiv.org/abs/1708.04182
Timing properties of black hole X-ray binaries in outburst can be modeled with mass accretion rate fluctuations propagating towards the black hole. Such models predict time lags between energy bands due to propagation delays. First application of a p
Externí odkaz:
http://arxiv.org/abs/1704.07705
The power spectrum of the X-ray fluctuations of accreting black holes often consists of two broad humps. We quantitatively investigate the hypothesis that the lower frequency hump orig- inates from variability in a truncated thin accretion disc, prop
Externí odkaz:
http://arxiv.org/abs/1607.08178
We present a spectral and timing analysis of the black hole candidate MAXI J1543-564 during its 2011 outburst. As shown in previous work, the source follows the standard evolution of a black hole outburst. During the rising phase of the outburst we d
Externí odkaz:
http://arxiv.org/abs/1403.2308
Akademický článek
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Autor:
Cannavò, L., Albano, D., Messina, C., Corazza, A., Rapisarda, S., Pozzi, G., Di Bernardo, A., Parafioriti, A., Scotto, G., Perrucchini, G., Luzzati, A., Sconfienza, L.M.
Publikováno v:
In Clinical Radiology September 2019 74(9):736-736
Akademický článek
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