Zobrazeno 1 - 10
of 4 039
pro vyhledávání: '"GIORDANO L."'
Autor:
Dipasquale, A., Franceschi, E., Giordano, L., Maccari, M., Barigazzi, C., Di Nunno, V., Losurdo, A., Persico, P., Di Muzio, A., Navarria, P., Pessina, F., Padovan, M., Santoro, A., Lombardi, G., Simonelli, M.
Publikováno v:
In ESMO Open June 2024 9(6)
Autor:
Filippi, C., Damioli, S., Accorsi, P., Crotti, E., Fazzi, E.M., Galli, J., Martelli, P., Morandi, A., Muda, A., Pinghini, S., Saottini, S., Sforza, S.E., Milito, G., Giordano, L.
Publikováno v:
In Seizure: European Journal of Epilepsy May 2024 118:47-52
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Autor:
Zugno, M., Tapparo, A., Colombini, M., Galimberti, G., Sacchi, S., Siena, F., Cavagna, B., Ciampitti, M., Giordano, L.
Publikováno v:
EPPO Bulletin; Aug2024, Vol. 54 Issue 2, p182-188, 7p
Autor:
Casa, R., author, Pascucci, S., author, Palombo, A., author, D’Urso, G., author, Maltese, A., author, Ciraolo, G., author, Giordano, L., author, Lopez-Lozano, R., author, Baret, F., author, Jones, H.G., author
Publikováno v:
Precision agriculture ’09. :47-54
Autor:
Freeland, E., Tran, K-V., Irwin, T., Giordano, L., Saintonge, A., Gonzalez, A., Zaritsky, D., Just, D.
We detect ionized gas characteristics indicative of winds in three disk-dominated galaxies that are members of a super-group at z=0.37 that will merge to form a Coma-mass cluster. All three galaxies are IR-luminous (L_IR > 4 x 10^{10} L_sun, SFR >8 M
Externí odkaz:
http://arxiv.org/abs/1111.0289
Giant low surface brightness galaxies (GLSBs) have flat discs extending up to ~100 kpc. Their formation is a puzzle for cosmological simulations in the cold dark matter scenario. We suggest that GLSBs might be the final product of the evolution of co
Externí odkaz:
http://arxiv.org/abs/0808.4101
We simulate the collisional formation of a ring galaxy and we integrate its evolution up to 1.5 Gyr after the interaction. About 100-200 Myr after the collision, the simulated galaxy is very similar to observed ring galaxies (e.g. Cartwheel). After t
Externí odkaz:
http://arxiv.org/abs/0710.5354
We report on the discovery of the z=1.016 cluster RzCS 052 using a modified red sequence method, followup spectroscopy and X-ray imaging. This cluster has a velocity dispersion of 710+-150 km/s, a virial mass of 4.0e14 Msol (based on 21 spectroscopic
Externí odkaz:
http://arxiv.org/abs/0710.1023
Chandra and XMM-Newton observations of the Cartwheel galaxy show ~17 bright X-ray sources (>~5x10^38 erg s^-1), all within the gas-rich outer ring. We explore the hypothesis that these X-ray sources are powered by intermediate-mass black holes (IMBHs
Externí odkaz:
http://arxiv.org/abs/0710.0780