... resolution[*]
The central density obtained with the continuum data reduces to $\sim $ $6\times10^5$  $\hbox{{\rm cm}}^{-3}$ when averaged within 26 $^{\prime \prime }$.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
...1989)[*]
The use of the relation found in L1544 by Caselli et al. (2002b) shifts the theoretical curves up by a factor of $\sim $1.3 in deuterium fractionation.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
...([*]
When D2H+ is included in the model, Eq. (4) becomes:

\begin{eqnarray*}R_{\rm deut} & \simeq
\frac{1/3 \left[\hbox{${\rm H}_{2}{\rm ...
...$ }\right]/\left[\hbox{${\rm H}_{3}^{+}$ }\right]\right)^2}\cdot
\end{eqnarray*}


.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
... center[*]
The linewidth toward the center and the observed $\Delta v$-b trend can also be matched assuming a central infall speed 1.5 times larger than the one calculated by CB in their model t3 and no extra broadening (e.g. turbulence) needs to be invoked. However, this is not consistent with the CB model at time t3 and we do not further discuss this possibility. On the other hand, recent ${\rm H}_{2}{\rm D}^{+}$ observations toward L1544 (Caselli et al. 2003) also imply larger central infall speed than predicted by CB-t3 (van der Tak et al. 2003).
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
Copyright ESO 2004