Issue |
A&A
Volume 543, July 2012
|
|
---|---|---|
Article Number | A59 | |
Number of page(s) | 21 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361/201219110 | |
Published online | 27 June 2012 |
Online material
Appendix A: Tables with photometry and SEDs
Ultraviolet, optical and near-IR photometry.
Mid-infrared photometry.
Sub-mm and mm photometry for a sub-sample of stars.
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Fig. A.1
SEDs of the stars in the sample. Triangles are photometric upper limits. For each panel, the best fit is the black-solid line and the models fitting with |
Open with DEXTER |
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Fig. A.1
continued. |
Open with DEXTER |
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Fig. A.1
continued. |
Open with DEXTER |
![]() |
Fig. A.1
continued. |
Open with DEXTER |
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Fig. A.1
continued. |
Open with DEXTER |
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Fig. A.2
Subsample of stars with fluxes available at λ ≥ 0.35 mm (log ν [GHz] ≤ 2.9, see Table A.3). The best graybody fits yielding the indicated values for tD and β are shown. Fluxes at λ ≤ 2.0 mm (log ν [GHz] ≥ 2.1) are weighted stronger in the fits. |
Open with DEXTER |
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Fig. A.2
continued. |
Open with DEXTER |
© ESO, 2012
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