C2D Spitzer-IRS spectra of disks around T Tauri stars - IV. Crystalline silicates

J. Olofsson; J.-C. Augereau; E. F. van Dishoeck; B. Merín; F. Lahuis; J. Kessler-Silacci; C. P. Dullemond; I. Oliveira; G. A. Blake; A. C. A. Boogert; J. M. Brown; N. J. Evans; V. Geers; C. Knez; J.-L. Monin; K. Pontoppidan

doi:10.1051/0004-6361/200912062

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Volume 507 / No 1 (November III 2009)

A&A, 507 1 (2009) 327-345

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Issue		A&A Volume 507, Number 1, November III 2009


Page(s)		327 - 345
Section		Interstellar and circumstellar matter
DOI		https://doi.org/10.1051/0004-6361/200912062
Published online		08 September 2009

Online Material

Table 4: Characteristics of the observations.

Table 5: Signal-to-noise ratios for detections of crystalline silicate features, amorphous silicate 10 $\mu$ m feature and silica.

$\begin{figure} \par\includegraphics[width=18cm,clip]{12062f20.ps} \end{figure}$	Figure 15: Spitzer/IRS spectra of young stars in the Perseus cloud, in units of Jy. Gray areas correspond to 3- $\sigma$ uncertainties as estimated in Sect. 2.4. Sources are sorted by increasing Right Ascension. Red color is for SL module, orange for SH, blue for LL and dark purple for LH.
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$\begin{figure} \par\includegraphics[width=18cm,clip]{12062f21.ps} \end{figure}$	Figure 16: Same as Fig. 15 but for the Taurus star sample.
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$\begin{figure} \par\includegraphics[width=18cm,clip]{12062f22.ps} \end{figure}$	Figure 17: Same as Fig. 15 but for the Chamaleon star sample.
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$\begin{figure} \par\includegraphics[width=18cm,clip]{12062f23.ps} \end{figure}$	Figure 18: Spitzer/IRS spectra for the Chamaleon sample: continued.
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$\begin{figure} \par\includegraphics[width=18cm,clip]{12062f24.ps} \end{figure}$	Figure 19: Same as Fig. 15 but for the Lupus star sample.
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$\begin{figure} \par\includegraphics[width=18cm,clip]{12062f25.ps} \end{figure}$	Figure 20: Same as Fig. 15 but for the Ophiuchus star sample.
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$\begin{figure} \par\includegraphics[width=18cm,clip]{12062f26.ps} \end{figure}$	Figure 21: Spitzer/IRS spectra for the Ophiuchus sample: continued.
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$\begin{figure} \par\includegraphics[width=18cm,clip]{12062f27.ps} \end{figure}$	Figure 22: Same as Fig. 15 but for the Serpens star sample.
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$\begin{figure} \par\includegraphics[width=18cm,clip]{12062f28.ps} \end{figure}$	Figure 23: Same as Fig. 15 but for the 3 isolated stars in our sample.
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$\begin{figure} \par\includegraphics[width=18cm,clip]{12062f29.ps} \end{figure}$	Figure 24: Same as Fig. 15 but for the 4 objects with spectra similar to C-rich and O-rich AGB stars.
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