\begin{table}%t2 \par \caption{\label{tab:tabices}Grain mantle compositions.} %\centerline {\begin{tabular}{llllllllll} \hline \hline%\\[-3mm] Species$^{a}$& \object{Elias 16}$^{b}$& \object{Elias 29}$^{c}$ & Class \rm{I}/\rm{II} Objects$^{d}$ & Model &$t = 0.0$ &$t = 0.5$ $t_{{\rm ff}}$ &$t = 1.5$ $t_{{\rm ff}}$ &$t = 2.5$ $t_{{\rm ff}}$ & Midplane disk$^{e}$\\ \hline%\\[-3mm] \rm{H$_{2}$O}$^{f}$ & $100$ & 100 & 100&\rm{S} & $1.55(-4)$ & $1.65(-4)$ & $1.71(-4)$& $1.71(-4)$&$1.8(-4)$\\ & & & &\rm{G} & {\it 1.24(--5)} & {\it 8.29(--6)} & {\it 4.5(--6)} &{\it 4.2(--6)} & {\it 1.4(--5)}$^{g}$ \\ \rm{CO} & $25$ & 5.6 & \ldots &\rm{S} &13.9 & 17.0 & 11.6 & 5.0 & 17.6\\ & & & & \rm{G} &71.6& 61.1& 31.4 &13.5 &77.5\\ \rm{CO$_{2}$} & $24$& 22 & $\sim $12 &\rm{S}&46.9 &40.6&31.0&29.8&37.7\\ & & & &\rm{G}& 3.6(--1) & 3.1(--1)& 2.2(--1) & 2.2(--1) &4.2(--1)\\ \rm{CH$_{3}$OH} & $<$2.3 & $<$4.4 & $\ga$2--9 &\rm{S}&8.7&7.0&6.6&6.7&2.2 \\ & & & &\rm{G} & 1.4(--5) & 2.1(--5) & 2.9(--5) & 2.9(--5) & 7.0(--8) \\ \rm{NH$_{3}$} & $\leq $8 & $< $9.2 & $\la $14 &\rm{S}&$9.8(-1)$&$3.3(-1)$&$2.6(-1)$&$3.4(-2)$&$4.0(-1)$\\ & & & &\rm{G} & 1.7(--2) & 1.1(--2) & 2.7(--3) & 1.0(--3) & 6.0(--3) \\ \rm{CH$_{4}$} & $<$3 & $<$1.6 & $\sim$4&\rm{S} & $1.1(-1)$&$1.7(-1)$&$1.4(-1)$&$1.0(-1)$&1.8\\ & & & &\rm{G} & 2.2 & 2.0& 1.6 & 1.4 & 1.0 \\ \rm{H$_{2}$CO}& \ldots & $<$1.8& $\sim$2&\rm{S}&1.1&1.6&3.9&4.1&2.9\\ & & & &\rm{G} & 4.5(--4) & 3.7(--4) & 4.3(--4) & 4.7(--4) &4.8(--4) \\ \rm{OCS}& $< $0.2 & $<$0.05&\ldots&\rm{S}&$4.3(-9)$&$4.9(-10)$&$4.6(-10)$&$8.1(-10)$&$0$\\ & & & & \rm{G} &3.7(--3) & 4.0(--3) & 3.0(--3) & 2.7(--3) &9.1(--2) \\ \rm{HCOOH}& \ldots& $< $0.9& $\sim$0.6&\rm{S}&$1.5$&$2.6(-2)$&$1.4(-2)$&$1.4(-2)$&$3.4(-2)$\\ & & & & \rm{G} & 7.7(--3) & 9.3(--3) & 7.7(--3) & 7.1(--3) & 6.9(--1) \\ \rm{SO$_{2}$}& \ldots& \ldots& $\sim $0.5&\rm{S}&$2.3(-2)$&$1.3(-2)$&$8.7(-3)$&$8.4(-3)$&$1.2(-2)$\\ & & & &\rm{G} & 7.8(--4) & 1.0(--3) & 7.0(--4) & 5.9(--4) & 8.3(--3) \\ \hline \end{tabular}} \par \smallskip Observed ice compositions as percentage of the \rm{H$_{2}$O} abundance compared with model results. Every first line for a species shows the results from Model \rm{S} (includes surface reactions) and the second line shows the results for Model \rm{G} (excludes surface reactions). $^{a}$ Abundances are given as $a(b) = a \times 10^{b}$. $^{b}$ \rm{CO} \cite{1995ApJ...455..234C}; \rm{CO$_{2}$}, \rm{CH$_{3}$OH}, \rm{NH$_{3}$}, and \rm{CH$_{4}$} \cite{2005ApJ...635L.145K}; \rm{OCS} \cite{1997ApJ...479..839P}. $^{c}$ \cite{2000IAUS..197..135E} and \cite{2004ASPC..309..547B}. $^{d}$ \cite{2007arXiv0712.2458Z}. $^{e}$ At $t = 2.5$ $t_{{\rm ff}}$ and a radius of $\sim$500~AU. $^{f}$ \rm{H$_{2}$O} fractional abundance are given for the simulation: $n({\rm H}_{2}{\rm O})/n({\rm H}_2)$. $^{g}$ For model~\rm{G} we have taken an \rm{H$_{2}$O} fractional abundance of $1.8 \times 10^{-4}$ for calculating the ice fraction of other species, instead of the reported values on this line. \end{table}