Astronomy & Astrophysics

Table 7: Five candidate Class III sources from Table 3. These are probably in the transition phase between Class II and III having some remaining IR excess. K-band magnitudes for two sources are obtained from Kaas et al. (1995).
ISO Other ID $\alpha_{IR}^{7-14}$ ${\alpha _{IR}^{2-14}}$ $\alpha_{IR}^{2-7}$

#

112 -1.67

190 -1.98 -1.83 -1.73

210 -2.00

311 BD+01 3689B -1.73 -2.21 -2.54

332 -1.72

Identifier acronyms as in Table 3.

**Table 7:** Five candidate Class III sources from Table 3. These are probably in the transition phase between Class II and III having some remaining IR excess. K-band magnitudes for two sources are obtained from Kaas et al. (1995).
ISO	Other ID	$\alpha_{IR}^{7-14}$	${\alpha _{IR}^{2-14}}$	$\alpha_{IR}^{2-7}$
#
112		-1.67
190		-1.98	-1.83	-1.73
210		-2.00
311	BD+01 3689B	-1.73	-2.21	-2.54
332		-1.72

Source LaTeX | All tables | In the text