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 m feature and silica.
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Figure 15:
Spitzer/IRS spectra of young stars in the Perseus cloud, in units of Jy. Gray areas correspond to 3- |
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Figure 16: Same as Fig. 15 but for the Taurus star sample. |
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Figure 17: Same as Fig. 15 but for the Chamaleon star sample. |
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Figure 18: Spitzer/IRS spectra for the Chamaleon sample: continued. |
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Figure 19: Same as Fig. 15 but for the Lupus star sample. |
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Figure 20: Same as Fig. 15 but for the Ophiuchus star sample. |
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Figure 21: Spitzer/IRS spectra for the Ophiuchus sample: continued. |
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Figure 22: Same as Fig. 15 but for the Serpens star sample. |
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Figure 23: Same as Fig. 15 but for the 3 isolated stars in our sample. |
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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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