MBM 12: young protoplanetary discs at high galactic latitude

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Volume 497 / No 2 (April II 2009)

A&A, 497 2 (2009) 379-392

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Table 3:

Summary of the spectral appearance of the detected targets.
Object	SED^a	Enstatite^b	Forsterite^b
MBM 12-1	Photosphere	-	-
MBM 12-2	Full	-	19, 27.8, 33 $\mu$ m
MBM 12-3	TO candidate	9.3:	11.3:, 19:, 27.8, 33 $\mu$ m
MBM 12-4	Full	-	11.3:, 19:, 27.8, 33 $\mu$ m
MBM 12-5	Full	-	19, 27.8, 33 $\mu$ m
MBM 12-6	TO candidate	9.3 $\mu$ m	27.8, 33 $\mu$ m
MBM 12-10	TO candidate	9.3 $\mu$ m	23.4, 27.8 $\mu$ m
MBM 12-12	Full	9.3 $\mu$ m	11.3, 19, 27.8, 33 $\mu$ m

^a We distinguish between a ``full'' and a ``transitional'' disc, based on the presence or absence of excess emission at wavelengths shorter than 8 micron, and write ``transitional object (TO) candidate'' when this classification needs to be confirmed by additional photometry.
^b We list the wavelengths at which features of enstatite and forsterite are present. Colons indicate uncertain detections.

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