LEADER 01802nam 22005413 450 001 9910130517003321 005 20091113000000.0 035 $a(CKB)3400000000020096 035 $a(ItFiC)it 02414043 035 $a(SSID)ssj0001456753 035 $a(PQKBManifestationID)12576862 035 $a(PQKBTitleCode)TC0001456753 035 $a(PQKBWorkID)11429730 035 $a(PQKB)10587314 035 $a(EXLCZ)993400000000020096 100 $a20101102d2009 uy 0 101 0 $afre 181 $ctxt 182 $cc 183 $acr 200 00$aSociété et climats dans l'Empire romaine $epour une perspective historique et systémique de la gestion des ressources en eau dans l'Empire romain /$fsous la direction de Ella Hermon ; préface de Luigi Labruna 210 $aNapoli $cEditoriale scientifica$d2009 215 $axv, 519 p. $cill. ;$d24 cm 300 $aProceedings of the meeting held in Laval, Canada, Nov. 18-20, 2008. 300 $aTexts in English, French or Italian. 311 $a88-6342-117-X 320 $aIncludes bibliographical references. 517 $aSociété et climats dans l'Empire romaine 606 $aClimate and civilization$zRome$vCongresses 606 $aEarth & Environmental Sciences$2HILCC 606 $aMeteorology & Climatology$2HILCC 607 $aRome$xClimate$vCongresses 615 0$aClimate and civilization 615 7$aEarth & Environmental Sciences 615 7$aMeteorology & Climatology 676 $a937 676 $a551 676 $a333 676 $a340 676 $a306 676 $a304 702 $aHermon$b Ella 801 0$bItFiC 801 1$bItFiC 906 $aBOOK 912 $a9910130517003321 996 $aSociété et climats dans l'Empire romaine$92429076 997 $aUNINA LEADER 03039nam 2200673 a 450 001 9910782802703321 005 20230721021141.0 010 $a1-383-04518-6 010 $a1-282-05333-7 010 $a9786612053337 010 $a0-19-156280-7 035 $a(CKB)1000000000747337 035 $a(EBL)431188 035 $a(OCoLC)320052141 035 $a(SSID)ssj0000218249 035 $a(PQKBManifestationID)11191114 035 $a(PQKBTitleCode)TC0000218249 035 $a(PQKBWorkID)10212868 035 $a(PQKB)11464970 035 $a(Au-PeEL)EBL431188 035 $a(CaPaEBR)ebr10288472 035 $a(Au-PeEL)EBL4786690 035 $a(CaONFJC)MIL205333 035 $a(Au-PeEL)EBL7039289 035 $a(MiAaPQ)EBC431188 035 $a(EXLCZ)991000000000747337 100 $a20081117d2009 uy 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 10$aParticle astrophysics$b[electronic resource] /$fD.H. 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