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Table 3

New spectroscopic data of stars and brown dwarfs in σ Orionis.

Name Sp. EW(Ca K) EW(Ca H) EW(Hγ) EW(Hβ) EW(Hα) EW(Li i) SED
type [Å] [Å] [Å] [Å] [Å] [Å] classa

Mayrit 783254 K0: +13  ±  2 +9  ±  2 +0.7  ±  0.2 +0.8  ±  0.6 +0.8  ±  0.2 +0.62  ±  0.15 III
Mayrit 528005 AB K7.0  ±  1.0 +4.5  ±  0.2 +4.5  ±  0.4  <+0.4  <+0.2 –1.9  ±  0.2 +0.6  ±  0.2 II
Mayrit 609206 K7.0  ±  1.0e –26  ±  3 –26  ±  3 –9  ±  2 –15.0  ±  1.0 –46  ±  2 +0.45  ±  0.15 II
Mayrit 957055 M0.0  ±  1.0 –13  ±  2 –12  ±  2 –3.5  ±  1.5 –3.5  ±  0.5 –5.5  ±  0.3 +0.65  ±  0.15 III
Mayrit 180277 M1.0  ±  1.0 –7  ±  2 –8  ±  2 –2.5  ±  1.5 –3.0  ±  1.0 –4.4  ±  0.2 +0.60  ±  0.15 III:
Mayrit 156353 M1.0  ±  1.0 –10  ±  2 –9.5  ±  1.0 –2.0  ±  0.5 –2.5  ±  0.2 –3.9  ±  0.2 +0.55  ±  0.15 II
Mayrit 662301 M1.0  ±  1.0e –5.5  ±  1.5 –5.5  ±  1.0 –9  ±  2 –7.0  ±  1.0 –11.8  ±  0.9 +0.55  ±  0.10 II
Mayrit 1298302 M3.0  ±  0.5  >–2.0  >–2.0  >–1.0 –2.6  ±  0.2 –3.5  ±  0.3  <+0.2 III:
Mayrit 872139 M5.5  ±  1.0 ... ... ... ... –13  ±  3  <+1.0 III
Mayrit 1196092 M6.0  ±  1.0e ... ... ... ... –125  ±  15  <+1.0 II

Notes. 

(a)

Spectral-energy-distribution class: “II”: with a disc; “III”: without a disc; “III:”: probably without a disc.

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