Zobrazeno 1 - 10
of 716
pro vyhledávání: '"Toscano E"'
Publikováno v:
Advances in Medical Education and Practice, Vol 2012, Iss default, Pp 55-60 (2012)
Fabrizio Consorti, Mariagiovanna Notarangelo, Laura Potasso, Emanuele ToscanoDepartment of Surgical Sciences, Faculty of Medicine and Dentistry, University Sapienza of Rome, Rome, ItalyAbstract: Developing and assessing professionalism in medical stu
Externí odkaz:
https://doaj.org/article/8b3b8d45bd8f44bd840c08e5c55ca444
Autor:
Suárez-Soto, E., Peris-de la Hoz, A., Sanchez-Fernandez-Quejo, A., Rodriguez-Toscano, E., Lagunas, N., Reneses, B., De la Torre-Luque, A.
Publikováno v:
In The European Journal of Psychiatry January-March 2025 39(1)
Publikováno v:
In Medicine - Programa de Formación Médica Continuada acreditado October 2020 13(19):1061-1071
Publikováno v:
In Medicine - Programa de Formación Médica Continuada acreditado October 2020 13(19):1104-1108
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
Mon.Not.Roy.Astron.Soc. 357 (2005) 295-303
Super-Eddington accretion discs with 3 and 15 dot M_E around black holes with mass 10 M_sun are examined by two-dimensional radiation hydrodynamical calculations extending from the inner disc edge to 5*10^4 r_g and lasting up to \sim 10^6 r_g/c. The
Externí odkaz:
http://arxiv.org/abs/astro-ph/0411743
It is well known that the rotating inviscid accretion flows with adequate injection parameters around black holes could form shock waves close to the black holes, after the flow passes through the outer sonic point and can be virtually stopped by the
Externí odkaz:
http://arxiv.org/abs/astro-ph/0403115
Publikováno v:
Mon.Not.Roy.Astron.Soc.351:297,2004
We show that accretion disks, both in the subcritical and supercritical accretion rate regime, may exhibit significant amplitude luminosity oscillations. The luminosity time behavior has been obtained by performing a set of time-dependent 2D SPH simu
Externí odkaz:
http://arxiv.org/abs/astro-ph/0309094
Publikováno v:
Mon.Not.Roy.Astron.Soc.348:361,2004
We show that a standard Shakura-Sunyaev accretion disc around a black hole with an accretion rate lower than the critical Eddington limit does show the instability in the radiation pressure dominated zone. We obtain this result performing time-depend
Externí odkaz:
http://arxiv.org/abs/astro-ph/0307480
Autor:
Jones, -->A.C., Toscano, E., Botting, N., Marshall, C.-->R., Atkinson, J.R., Denmark, T., Herman, -->R., Morgan, G.
Publikováno v:
In Research in Developmental Disabilities December 2016 59:268-282