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Table 4.

Strongly accreting stars and brown dwarfs with EW(Hα) < –50 Å.

Mayrit Alternative Hα emitter Variable SpT EW(Hα) Remarks
name name name adopted [Å]
Mayrit 1329304 Haro 5-5 Haro 5-5 ... M2.5 –118 EW(Li I) this work;
red-shifted Hα
Mayrit 873229AB Haro 5-7 ESO-Ha 1646 NSV 2489 M4.5 –59 Red-shifted Hα
Mayrit 757219 Haro 5-8 Kiso A-0976 322 SVS 1241 M1.0 –91
Mayrit 329261AB [SWW2004] 207 ... ... M4.5 –148 EW(Hα) this work
Mayrit 1207349 Haro 5-9 Kiso A-0976 330 V2731 Ori M0.0 –54
Mayrit 1316178 S Ori J053847.2–025756 ... ... M6.5 –80 EW(Hα) this work
Mayrit 687156 [WB2004] 26 ESO-Ha 1693 ... M4.5 –50 EW(Li I) this work;
red-shifted Hα
Mayrit 871071 Haro 5-27 Kiso A-0976 356 V510 Ori K2 –123 Source of HH 444
Mayrit 1279052 Haro 5-30 Haro 5-30 ... M5.5 –100
Mayrit 1041082 Haro 5-32 Kiso A-0976 359 V604 Ori M3.0 –89 Blue-shifted Hα
Mayrit 1196092 S Ori J054004.5–023642 ... ... M6.5 –125 EW(Li I) this work;
brown dwarf
Mayrit 1364078 V2754 Ori ... V2754 Ori M6.5 –73
... Haro 5-40 Kiso A-0976 375 ... M4.0 –147 EW(Hα) this work; IC 434
... Haro 5-44 Kiso A-0904 111 V612 Ori M3: –160 EW(Hα) this work;
red-shifted Hα; IC 434

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