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Table 7
Tentative spectral classification of the low mass stars in our sample, based on the relative strength of CO (6, 3) 16198 Å, Brγ, and CO (2, 0) 22 957 Å.
No. | Relative strength | Spectral classification |
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38 | Strong CO (6,3); No Brγ; Strong CO (2,0) | Early MIII |
78 | Weak CO (6,3); Weak Brγ; Strong CO (2,0) | Late G III |
158 | Weak CO (6,3); Strong Brγ; Strong CO (2,0) | Early/mid GI-III |
396 | Medium CO (6,3); No Brγ; Strong CO (2,0) | Mid/Late KI-III |
437 | Weak CO (6,3); Strong Brγ; Medium CO (2,0) | Early GI-III |
694 | Medium CO (6,3); Strong Brγ; Medium CO (2,0) | Early KI-III |
881 | Strong CO (6,3); Weak Brγ; Strong CO (2,0) | Late K/Early MI-III |
1059 | No CO (6,3); No Brγ; Medium CO (2,0) | Early MV |
1128 | No CO (6,3); Strong Brγ; Medium CO (2,0) | GV |
1203 | Medium CO (6,3); No Brγ; Strong CO (2,0) | Mid/Late KI-III |
1358 | Weak CO (6,3); Weak Brγ; Medium CO (2,0) | Early KV |
1374 | Weak CO (6,3); Medium Brγ; Weak CO (2,0) | Late G/Early KV |
1379 | No CO (6,3); Strong Brγ; Weak CO (2,0) | Mid GIII |
1408 | Strong CO (6,3); No Brγ; Strong CO (2,0) | KIII |
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