01239nam0 22003253i 450 TER001181920231121125831.0888713246120220613d2006 ||||0itac50 baitaitz01i xxxe z01n˜Il œvolo della VespaCorradino D'Ascanio, dal sogno dell'elicottero allo scooter che ha motorizzato l'ItaliaSandro MarinacciL'AquilaTextusstampa 2006109 p.21 cm.˜La œmemoria6001TER00093752001 ˜La œmemoria6D'Ascanio, CorradinoFIRRMLC303273IMotocicliIndustriaItaliaFIRRMLC459751N629.2275Veicoli terrestri a motore, cicli. Motociclette e motorette22Marinacci, SandroTERV0020390701447410ITIT-0120220613IT-FR0017 Biblioteca umanistica Giorgio ApreaFR0017 NTER0011819Biblioteca umanistica Giorgio Aprea 52DGA E 100 52SBA0000278875 VMB RS A 2022061320220613 52Volo della Vespa3637331UNICAS02804nam 2200589z- 450 991055768420332120220111(CKB)5400000000044690(oapen)https://directory.doabooks.org/handle/20.500.12854/76813(oapen)doab76813(EXLCZ)99540000000004469020202201d2021 |y 0engurmn|---annantxtrdacontentcrdamediacrrdacarrierThe Physical Properties of the Groups of GalaxiesBasel, SwitzerlandMDPI - Multidisciplinary Digital Publishing Institute20211 online resource (250 p.)3-0365-1773-1 3-0365-1774-X Galaxy groups consist of a few tens of galaxies bound in a common gravitational potential and contain a significant fraction of the overall universal baryon budget. Therefore, they are key to our understanding of how the bulk of matter in the Universe accretes and forms hierarchical structures and how different sources of feedback affect their gravitational collapse. However, despite their crucial role in cosmic structure formation and evolution, galaxy groups have received less attention compared to massive clusters. This is perhaps in part due to their rarity in being observed and properly characterized. With the advent of eROSITA, many thousands of galaxy groups will be detected by X-ray, complementing optical and SZ coverage. In this Special Issue we collected and organized the latest developments in our understanding of these systems and present future prospects from both observational and theoretical points of view.Research and information: generalbicsscactive galactic nucleiactive nucleiblack holescosmological parameterselliptical galaxiesfossil galaxy groupsgalaxies:abundancesgalaxies:clusters:intracluster mediumgalaxy clustersgalaxy groupsgalaxy surveyshydrodynamical and cosmological simulationshydrodynamical simulationsintragroup medium/plasman/aUV observationsX-ray and optical observationsX-ray observationsX-rays:galaxiesResearch and information: generalLovisari Lorenzoedt1300053Ettori StefanoedtLovisari LorenzoothEttori StefanoothBOOK9910557684203321The Physical Properties of the Groups of Galaxies3025377UNINA