Issue |
A&A
Volume 578, June 2015
|
|
---|---|---|
Article Number | A23 | |
Number of page(s) | 16 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361/201424073 | |
Published online | 29 May 2015 |
Online material
Class II objects detected by Herschel in the Lupus clouds.
Herschel photometry for the 34 YSOs detected in the maps.
Normalized flux densities of the median SED, lower SED (first quartile), and upper SED (fourth quartile) of the Class II objects in Lupus I, III, and IV.
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Fig. 3
SEDs of the 29 YSOs with Herschel detections that do not fulfill our transitional disk selection criteria. |
Open with DEXTER |
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Fig. 3
continued. |
Open with DEXTER |
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Fig. 4
Images of each of the 34 sources with at least one point source detected by Herschel, plus object 2MASSJ1608537, added for completeness. The images correspond to a box of 120′′ × 120′′ in size. Coordinates are given in Table 5. The color scale is defined with the root-mean square of the pixel values (as background level) and this number plus three times the standard deviation (as maximum level). North is up and east is left. A circle indicates the expected position of the target. The standard deviation computed around the sources is shown for each image (bottom right). |
Open with DEXTER |
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Fig. 4
continued. |
Open with DEXTER |
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Fig. 4
continued. |
Open with DEXTER |
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Fig. 4
continued. |
Open with DEXTER |
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Fig. 4
continued. |
Open with DEXTER |
© ESO, 2015
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