Does Drosophila suzukii represent an additional factor of risk of sour rot disease development in wine grape?
3
0
0
Testo completo
(2) 45346 534356. 8 9 6656 !. 664"4#6 $846546%5464&434356' 8365646%446466. 3445%#4654 () * 465* (+' &6$5'84! . ,2- . -. . /01231456789:5;<=>=1?1054@9AB5C535@4D:E41F4@GG5HIA1J1FAD@JC531K4D5L@2@F5G529M14/K39@A2@7J5NF4ADKJ9K4@J/8395G3 .
(3) 123416242789 4
(4)
(5) 996376343 992 262694 242
(6) 662943 4333 2739936 73. !" ## $%" &' () & $* ++ ,,( --&$( &+" &'.&+" $/ ," 0 --& $ 1 2 3* 2 &/ ,4 3$5 & ,165 #&$/ 4)&067 #& 8 9:;<=>8<?@ABC>8=D:;C>8EBC8<:F=D8EG=DA;<H8I?@DBAJAKL8I;EB<M?;8N?B=;?>89ABCEO:AB?8PCQGBC8RE@D>8S:E8 TUVWXUYZ[\]Y^_Y`ab^bYc[XYZd\]efeY[ffghUdieYjklm_Yno[fpqYrsWto]Y[XUYrdro]Y[Wo]stuvYwex[toVeXoYsrY yG<=E:BEzJ?8P@A<L<=?Q<8EBC8{:A;?<AG;@?<>8|?<?E;@D8EBC8}BBA~E=:AB8N?B=;?>89ABCEO:AB?8PCQGBC8 Z[\]_Y`ab^bYc[XYZd\]efeY[ffghUdie_Yno[fpqYrsWto]Y[Wo]stvYeXoetYhitd\WfoWteYssUYTXdtsXVeXoY jhTm_YXdetudopYsrYkteXos_Y`ab^bYcYZd\]efeY[ffghUdK?8I >8}=EJL8<?~?B=D8EBC8?:KD=8EG=DA;<H8 ?E;=Q?B=8AM8A;=:@GJ=G;?>8;?KAB8y=E=?8B:~?;<:=L>88K8EBC8:M?8y@:?B@?<8{JCK8NA;~EJJ:<>8|8 >8y8 ¡¢£¤¥¦§¨£©¢¤§¥ª8. Ì 4) 4)#3. Í Ã§¸¨£ª¨¢ ¨µ¨ª¨£¦¶ ª¨£¦¹¢¸¨¶¹®¨µ£ ¨£ª§¶¹ µ¢¤ Í ¬°±¤£¶¸¤ª¨¨¢¤¨¨¦£ » ¨£¤µ£¦¤µ ¦£ª¨¢ ¨µ¨ª»ª§¢¨ ¬°±£¢ ªª¨£ ¤£Êµ¤·¹ ¨µ¨ª¨£ª§¤µ ª Í Á£ª¤ª¶ µ¤§ µ ¤ª¶ª¨ ¨µ¨ª»¸££¤ ¨¢¬°±£¢ ªª¨£. «62
(7) 92. ¬¨ªª®£¦¨ ¨§¯¬°±²;A<AD:JE8<GOG³::¯´ª µµ² ¦¨¶ ªªª¤·£¦ ¸¨µ ¶¹¤¨ £¤µ¦¸£¥¬°±¤£¹¦¦ ¨£µ£®¨µ£££¦®£¦ ¶ ¥ºª§¨µ¦§®£¦ £¨ ª¤ £¨ª¹ µª¢¨¬°±¨µª¨£¸¨£ª» ª§¢¹¤£¢»¨¸¨ ª£¸¨ª¨µª ¨£®£¦ ¯º £ª¥»¼½¾¿²¥À¸¨ ª¨£ £ª£ ª¹£¤ µ£¦ª§££¦¨£ ¤¨ªª¨§¹ ¨¨¦¤¤§£¦ ¨¤¤µ£¦ µ£¦¦¶¹¸¨£ª»¥¥£¤ £ µ¦¤¨£ª£ª»¤ ¨¢¤ª¹¸ £ ·£ £ªª¨£¢¨¤¯Á¨ªªª¥»¼½¾¿²¥Â¦§¨µª¨£ ¨¢8<GOG³::¨ª£ª¹ £ª¨£®£ ¦ µ£¦ª§§¸ ª¨¹ µª£ ¦£¢¤£ª ·¤¨£ £¦ª§¸¤ª¨£¦¨¢ ¨¦ ¶¤ª¥Ã¨ ª§ §¹¨ª§ »¶¨ª¨¹¶¨ ¹ ®¢¨ª¨ ª§¤ªµ¶ª¹ ¨¢¬°±ª¨¸¤ª¨ ¨¦¶¤ªª¨£ª¤ª®£¦£ª¨ª¦¦ ¨µ¨ª ¸¨£ª¥. Ä 369 3824. 縪 »Å£¨ª£¨»¬¤§¸£Æ¶£ª µ¸¦£¨£ª§£ª¤ª¨¦ ª ¶ ®¨¢¢ ¨¸¨ ª¨£ µ¶ ªªª¨¬°±µª ¢¨¶¤¨¨£¹¥¬°±¢ §¸¶£ ¸¨µ ¹·ª¢¨ª®¨¹ £¤¦£¤¨£ª¤ª®ª§¤¨ªª¨£¦£ª®ª§ µ £ ¨£¨¢ ¶¤ªª¨ªª§¤¹£¦¶¤ª¨ ª¨ª§ª £ª¨£¬°±ª£¸£¹¥º¢ª ǹ »¬°±µª µ¸¸£¨¸¨ ª¨£¨£¶ ® »ª§¢ ®¨¸®§ ª§¦¶ §¸¶£¢µª§·ª£ª§ ª¤¶¨È µ£¤¨£ª¨¤ª¤ ¤¨£ª¨£ ¢¨¾½¹ ¥É ®ª§£¤ §£ª§§¨¨¦£ ª ®¨ ª¨£ª¨ ªÅªª ¤¨£ª££¦¨ ¹£ª§ª¤¦¨®ª§ª¨¢¨Êµªª¸£Êµ£ªªª¸ ¤§¤ª ª¨£¨¢¤¨¢¨¸¨¨£ª§¦¶ ¥Ë¨ª¤ª¹¸µ ¨¢ª§ ¶ ¦ ¨¢¤§¸ª¹® £¤¨£ ££¤ª¨¨¢ ¨µ¨ª£¤£ª ¸¨£ª¥Ã¨¤¨£¢¶¨ª¨¹ µª »£ª¢¤¬°±£¢ ªª¨£¨¢¶¦¦¦¤µ ª ¨¢.
(8) 1234561789 427989
(9) 3 3 315712 338739 7123 31 874387 7179 5 3531 69 896383631
(10) 9 3896591391237. 36917 27
(11) 712 54179431749478691763 4 73 3. !"#$!$% & %'#!!. (3 561 3 1 9131291 )*498341 769+39413 7912 5+2419419, 337+ 99+33. 73 5. 1383633495 34197917
(12) 533. 73 974 719 1 9 134197913 )*-
(13) 27427 37913 769+39413 79 99+3 73413 3. 73 . 383 -
(14) 276387 71771941 53. 73
(15) 9 19 5747314717. 1 7++3 7+ 5. 1383631-123 5443 78369 8963836314 1715139971796
(16) 9. 397+ 769+39413 79 5429 /0123450216 7
(17) 73+ 93 5 7+12329 83 13 7)3 96 3 1 9131253 41 66369 91 97364717 -129174569178373 1917
(18) 712 )*94 345178369 896383631
(19) 7127+ 933. 73 49 1312374 39 3943174 8691763 -9 977491 74 39 3 5. 163836 7
(20) 383 -
(21) 312781291123 3 343 )* 9::;<=><?@9<:ABC9<D9AA=9;<=;<>E?<FC9A<;9G<B><=;;H9<IEA<?@9<J=>9<:AEJ9A;K<CAEL=M9M<9::<NBO=>:<B>M< 5443 78369 8963836311495 3 87 515 3 1291 1374 +97 73417 123123 29- 743 5+ 933. 73 9 363 5 431763112338363174 719 9 47913
(22) 712 5. 19 769+3-953 941 93417+ 87713+ 71P 97966-
(23) 7133 915 3-7 39 3 -7 3413 1 -871745615 96 9417 3 -314Q49 1 +6765343+ 9374 719 12919 3 79 76 3 763 383631+ 93 5. 1. R S #& !!. T 63.U3196VWXYZ89 776+ 113)7+* 2769P[63\3]^_`5a\bcbd__Qe9+696 3 3417839515 3 7 7173 f5 963 1 47343ggehijkhjh Z 79117l3196VWXY[63\3]^_`5a\bcbd__P*713 9e* 276793Q971 13179679411
(24) 73 + 93 5 7+29 83 171
(25) 46467913
(26) 73+ 93 5417 3+7 f5 96m474 m16+XWgPnQeXXhgkXXYY.
(27)
Documenti correlati
well-studied lenticular galaxy that is covered excellently well in the scientific literature. This is fundamental to test the methodologies, verify the results, and probe
We present photometric light-curves of the transiting extrasolar planets WASP-39b and WASP-43b obtained with three San Pedro Martir telescopes by using the
The distributions are significantly different and the fraction of relaxed objects is smaller in the Planck sample (52±4 per cent) than in X-ray samples (~=74 per cent)
I curatori della mostra erano spaventati dal dato di fatto che a quel tempo la Croazia fosse una repubblica jugoslava, come anche da un altro fatto fondamentale, ov- vero, che
1, we compare W0643’s TripleSpec spectrum to SpeX Prism Spectral Library standards using SPLAT ( Burgasser 2014 ; Burgasser & Splat Development Team 2017 ).. Using the
We have also verified whether different modeling could ac- count for the source complex emission; in particular, motivated by the observed flat photon index (which may be partly
cluster XLSSC 086 also contains a radio source within a red host galaxy at its centre, and we note the increase in number of blue galaxies between XLSSC 086 and the large
