Zobrazeno 1 - 10
of 1 274
pro vyhledávání: '"BELVEDERE G"'
Autor:
Licitra, G., Marino, V.M., Mangione, G., Belvedere, G., Difalco, A., Petriglieri, R., Caccamo, M. *
Publikováno v:
In Journal of Dairy Science November 2023 106(11):7515-7529
Publikováno v:
2013, MNRAS 429, Issue 2, p.1080-1087
In this paper, in the framework of the secondary infall model, the correlation between the central surface density and the halo core radius of galaxy, and cluster of galaxies, dark matter haloes was analyzed, this having recently been studied on a wi
Externí odkaz:
http://arxiv.org/abs/1212.6797
Autor:
Zaqarashvili, T. V., Belvedere, G.
Publikováno v:
Astrophys.J.663:553-559,2007
The weakly non-linear interaction of slow magnetoacoustic and torsional Alfven waves propagating along an unperturbed poloidal magnetic field in a stellar interior is studied in the high plasma beta limit. It is shown that slow magnetoacoustic waves
Externí odkaz:
http://arxiv.org/abs/astro-ph/0703206
We discuss the mean-field dynamo action in protoneutron stars that are subject to instabilities during the early evolutionary phase. The mean field is generated in the neutron-finger unstable region where the Rossby number is $\sim 1$ and mean-field
Externí odkaz:
http://arxiv.org/abs/astro-ph/0603034
Publikováno v:
Astrophys.J.629:1164,2005
A magnetic flux tube may be considered both as a separate body and as a confined field. As a field, it is affected both by differential rotation ($\Omega$-effect) and cyclonic convection ($\alpha$-effect). As a body, the tube experiences not only a b
Externí odkaz:
http://arxiv.org/abs/astro-ph/0509828
Autor:
Zaqarashvili, T. V., Belvedere, G.
Publikováno v:
Mon.Not.Roy.Astron.Soc.Lett.362:L35-L39,2005
We suggest that the observed long-period Alfv{\'e}n waves in the solar wind may be generated in the solar interior due to the pulsation of the Sun in the fundamental radial mode. The period of this pulsation is about 1 hour. The pulsation causes a pe
Externí odkaz:
http://arxiv.org/abs/astro-ph/0506757
We have investigated the turbulent mean-field dynamo action in protoneutron stars that are subject to convective and neutron finger instabilities during the early evolutionary phase. While the first one develops mostly in the inner regions of the sta
Externí odkaz:
http://arxiv.org/abs/astro-ph/0504328
Publikováno v:
Astrophys.J. 579 (2002) 810-816; Erratum-ibid. 591 (2003) 498
We suggest a mechanism for enhancing magnetic activity in tidally interacting binaries. We suppose that the deviation of the primary star from spherical symmetry due to the tidal influence of the companion leads to stellar pulsation in its fundamenta
Externí odkaz:
http://arxiv.org/abs/astro-ph/0210222