Zobrazeno 1 - 10
of 373
pro vyhledávání: '"Falco, V. A."'
We study the contributions to the relativistic Fe $K_{\alpha}$ line profile from higher order images (HOIs) produced by strongly deflected rays from the disk which cross the plunging region, located between the innermost stable circular orbit (ISCO)
Externí odkaz:
http://arxiv.org/abs/2104.07707
Autor:
Papitto, A., Falanga, M., Hermsen, W., Mereghetti, S., Kuiper, L., Poutanen, J., Bozzo, E., Ambrosino, F., Zelati, F. Coti, De Falco, V., de Martino, D., Di Salvo, T., Esposito, P., Ferrigno, C., Forot, M., Götz, D., Gouiffes, C., Iaria, R., Laurent, P., Li, J., Li, Z., Mineo, T., Moran, P., Neronov, A., Paizis, A., Rea, N., Riggio, A., Sanna, A., Savchenko, V., Słowikowska, A., Shearer, A., Tiengo, A., Torres, D. F.
In the last 25 years, a new generation of X-ray satellites imparted a significant leap forward in our knowledge of X-ray pulsars. The discovery of accreting and transitional millisecond pulsars proved that disk accretion can spin up a neutron star to
Externí odkaz:
http://arxiv.org/abs/2012.01346
Autor:
Li, Zhaosheng, De Falco, V., Falanga, M., Bozzo, E., Kuiper, L., Poutanen, J., Cumming, A., Galloway, D. K., Zhang, Shu
Publikováno v:
A&A 620, A114 (2018)
SAX J1748.9-2021 is a transiently accreting X-ray millisecond pulsar. It is also known as an X-ray burster source discovered by Beppo-SAX. We analysed the persistent emission and type-I X-ray burst properties during its 2015 outburst. The source vari
Externí odkaz:
http://arxiv.org/abs/1810.05490
IGR~J18245--2452/PSR J1824--2452I is one of the rare transitional accreting millisecond X-ray pulsars, showing direct evidence of switches between states of rotation powered radio pulsations and accretion powered X-ray pulsations, dubbed transitional
Externí odkaz:
http://arxiv.org/abs/1704.04181
Akademický článek
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Autor:
De Falco, V., Kuiper, L., Bozzo, E., Galloway, D. K., Poutanen, J., Ferrigno, C., Stella, L., Falanga, M.
IGR J00291+5934 is the fastest-known accretion-powered X-ray pulsar, discovered during a transient outburst in 2004. In this paper, we report on Integral and Swift observations during the 2015 outburst, which lasts for $\sim25$ d. The source has not
Externí odkaz:
http://arxiv.org/abs/1611.08218
Publikováno v:
In ESMO Open June 2021 6(3)
Autor:
Garcia-Vidal, C., Sanchez-Rodriguez, I., Simonetti, A.F., Burgos, J., Viasus, D., Martin, M.T., Falco, V., Carratalà, J.
Publikováno v:
In Clinical Microbiology and Infection September 2017 23(9):653-658
Autor:
García-Díez, J., Alheiro, J., Pinto, A.L., Soares, L., Falco, V., Fraqueza, M.J., Patarata, L.
Publikováno v:
In Food Control January 2016 59:262-270
Autor:
Burgos, J., Falcó, V., Borrego, A., Sordé, R., Larrosa, M.N., Martinez, X., Planes, A.M., Sánchez, A., Palomar, M., Rello, J., Pahissa, A.
Publikováno v:
In Clinical Microbiology and Infection April 2013 19(4):385-391