Table 5: Summary of the spectral and photometric properties of the well studied objects as discussed in Sect. 4. Column 1: object name; Col. 2: spectral type; Cols. 3-6: spectral features detected in their K-band spectra; Cols. 7 (J - K) value, dereddened for foreground extinction; Col. 8: absolute, dereddened K-band magnitude; Col. 9: references: G87: Geballe & Persson (1987), C89: Carr (1989), C93: Chandler et al. (1993), C95: Chandler et al. (1995), vdA00: van den Ancker et al. (2000), S83: Scoville et al. (1983), L04: Lenorzer et al. (2004), vdA04: E02: Eiroa et al. (2002), van der Ancker (2004), C00: Clark & Steele (2000), D94: Dougherty et al. (1994), M88: McGregor et al. (1988), M96: Morris et al. (1996), V99: Voors (1999). $\dagger $: These values are for the B[e] supergaints.
Object/ Sp. Type Br$\gamma $ Pf HeI CO MgII/FeII E(J - K) K References
Object type                  
S106 O6-O8 V + + - + - 0.6 -5.4 G87, C89, C93, C95, vdA00
BN B0.5V + - - + + - - S83, G87, C89
NGC 2024-IRS2 B0V + + - + + 0.9 -7.0 G87, C93, C95, L04
Herbig Ae F - late B + - - - - 1.5 2 - -2 E02, vdA04
Herbig Be B + ? + some - 2-6 -1--5 E02, vdA04
Be B + + some - some 0.0-0.6 0--3 D94, C00
B[e] B + + some + + 2-6$^\dagger$ -6--10$^\dagger$ M88,M96,V99


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