Near-infrared low-resolution spectroscopy of Pleiades L-type brown dwarfs

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Table 3:

Luminosities, effective temperatures, and masses for our Pleiades targets.
Object	SpT	$\log{L/L_{\odot}}$	$T_{\rm eff}$	M
		(dex)	(K)	( $M_{\odot}$ )
PPl 1	M6.5 $\pm$ 0.5	-2.90 $\pm$ 0.04	2676 $\pm$ 120	$\sim$ 0.074
Calar 3	M8.0 $\pm$ 0.5	-3.18 $\pm$ 0.04	2584 $\pm$ 100	$\sim$ 0.054
Teide 1	M8.0 $\pm$ 0.5	-3.24 $\pm$ 0.04	2584 $\pm$ 100	$\sim$ 0.052
BRB 17	L0.0 $\pm$ 1.0	-3.68 $\pm$ 0.06	2350 $\pm$ 100	$\sim$ 0.035
PLIZ 28	L0.0 $\pm$ 1.0	-3.76 $\pm$ 0.06	2350 $\pm$ 100	$\sim$ 0.033
PLIZ 35	L2.0 $\pm$ 1.0	-3.94 $\pm$ 0.06	2110 $\pm$ 180	$\sim$ 0.028
BRB 21	L3.0 $\pm$ 1.0	-3.95 $\pm$ 0.06	1950 $\pm$ 150	$\sim$ 0.028
BRB 23	L3.5 $\pm$ 1.0	-3.98 $\pm$ 0.06	1875 $\pm$ 150	$\sim$ 0.027
BRB 29	L4.5 $\pm$ 1.5	-4.14 $\pm$ 0.12	1735 $\pm$ 190	$\sim$ 0.024

Source LaTeX | All tables | In the text

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