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28 Sep 2006: 3 }x%$É-3 , uwv $m#A3. tu )ô$ & u -)B& v 1m-3@B@- / v xv #" v ')B&!@0$Ð)B"%@B!,)B-3 %$Y"%$£|) },A#)ô&3@ ÀÅ t ... vÅv $Ð)B@BA'"%@ v x-3",. )B'$Ð,@BA3E0"%$ v -!1, uwv ') v 1m-0&("%$E0)B ')B %&()B@ v )3x v!

19 Apr 2006: 0]B]B@uxG-N+?3TQGH+?IA-oxGH=?xRU>A]B@M1-N==?G4/2L<@Mr;T2R2]t+;-N=B+?G4x143]B=.-N2_3T"G4/"=?3]B@M/U-0/,y14@ ... t+?36=?@MG4TU-01|-0/2Tx@M>36+.-N=B5;-N=B+?G4x143]T2R23!@)@5S/,?G4/2L0Õ@0z_3=B+?]B@0/i1HG4LMI,KTS=.-0LS9X@M>3a@MrP+?I23]B3!p0-

19 Apr 2006: #"%$$&' () ,.-.&/ 010 "%$$& 243 56 789 #:;,=<>;,@?" "'. A B!CEDGFIHKJ L=MNFPOQCSRTFIUVBWOTUVB!XYBZD[FM]T_TO BaDGFIBcbdUeJ fUgDh_ikjmlgDh_QCnB. ... Pea37fR$OaqPea4o4WdR$oBbBPeoq¢oqW)F,x;x'GF

19 Apr 2006: dashed red line;Model B’ – a flat distribution with r3 as a dashed blue line. ... For the inner part ofthe disk (r 350 AU), Model A/A’ and Model B/B’ givesimilar results, but Model A and A’ give a much betterfit for r >350 AU.

19 Apr 2006: W99 ignore the e†ects of radiation pressure,assuming, in e†ect, that large, dynamically stable dustgrains, with b B 0, orbit HR 4796A ; b is the ratio of theradiation pressure ... As discussed in 6, themid-infraredÈemitting particles, if they are

19 Apr 2006: ¢YKHz6VOzx{K.{{K!lzâZ}z]}¡!zC{B{B!6x$!z¢'! KzK!¡6 |6{K,.z{K.}z].{B6!x{#=!zVH{Kx/K6 ... K7K6},!{KHz66z6|z}¡!6H{K!}¡z/}zZh.B{K K}zC{K}¡xx{K!

19 Apr 2006: a@ a(1 [ b)/[1 [ 2b(1 ] e cos f )/(1 [ e2)] , (19). ... Of these large particles,only those with su†er no signiÐcant P-R drag evo-b b.

19 Apr 2006: F! a! TS- '4( );V! (Y C( E5[- M(&? 3$ (49 P#-# -;9!9]%& W5[- ; ) Ea'-'; UG4?3$ )9&$ B ; B- t%3 ,:E# ;! 5- t(&$7C0:; P B 'RS! ... G. u= K G %' àõö>øEàù ú»s6ø 6þC.ø?»ý ø @2& B B- u 7:>- ra%. (&

19 Apr 2006: 35! Q ,!6 J 3$, $6"8 )0 4" 4 JLKNK 4 B)!B";1G0 83f("E"8,! ... 8g)! =)! Q83I -!>," $' $-"8<=1)6,,-<=2RQ ]/-!SQ TU! 1L,!N 2 5%>=B- B.

27 Jul 2006: B, formerly Biomer; Free; Source Code; Java. Has moved from its old location to Professor David Case' group at the Scripps Research Institute.