Zobrazeno 1 - 10
of 118
pro vyhledávání: '"V. Zappala"'
Autor:
Mikhail Ya. Marov, G.M.F. A’Hearn, J. Baggaley, E. Bowell, S. Bowyer, D. Cruikshank, C. de Bergh, H. Keller, P. Lamy, V. Porubcan, J. Watanabe, I. Williams, V. Zappala
Publikováno v:
Transactions of the International Astronomical Union. 24:113-156
Autor:
Alessandro Morbidelli, Alberto Cellino, F. Migliorini, Mark E. Bailey, Brett Gladman, V. Zappala
Publikováno v:
Meteoritics & Planetary Science. 32:903-916
— A large body of evidence, including the presence of a dynamical family associated with 4 Vesta, suggests that this asteroid might be the ultimate source of both the V-type near-Earth asteroids (NEAs) and howardite, eucrite and diogenite (HED) met
Publikováno v:
Journal of neurosurgical sciences. 55(1)
Arteriovenous malformations (AVM) can occur in the entire central nervous system with a predilection of the supratentorial intracranial compartment. Intracerebral hemorrhage is the most common clinical presentation of AVM and associated with a high m
Autor:
V. Zappala, A. Cellino
Publikováno v:
Celestial Mechanics and Dynamical Astronomy. 54:207-227
Publikováno v:
Minerva anestesiologica. 64(9 Suppl 3)
The goal of the present multicenter, prospective, randomized clinical investigation was to compare the clinical efficacy and safety of sevoflurane and isoflurane during maintenance of and recovery from general anaesthesia in adult patients.With the a
Autor:
Z. Knezevic, V. Zappala
Publikováno v:
Icarus. 65:122-128
The Amplitude-Magnitude (AM) method is used for the pole determination of the asteroid 511 Davida, using observations from six oppositions. The possible North poles are found to be λ 1 = 92° ± 7°; β 1 = 33° ± 6°, and λ 2 = 303° ± 4°; β 2
Publikováno v:
The Moon and the Planets. 28:251-258
In the set of small satellites of Saturn recently imaged by the Voyager probes, we can observe the transition from irregularly-shaped, strength-dominated objects to larger, gravity-dominated bodies with shapes roughly fitting the theoretical equilibr
Publikováno v:
Icarus. 55:236-244
Photoelectric lightcurves of six asteroids, observed at the ESO 50-cm photometric telescope, are presented. 45 Eugenia, observed for pole determination program, showed a small amplitude of light variation, i.e., about 0.09÷0.10 mag. For 120 Lachesis
Autor:
V. Zappala’
Publikováno v:
Highlights of Astronomy. 8:273-279
Asteroid families are considered for the most to represent fragments of collisional breakup of precursor bodies. If true, this offers the unique possibility to examine the interiors of large bodies and to study the processes of collision on a scale m