Abstract
We report the detection of an Hα flare on the low-luminosity M9. 5 dwarf BRI 0021-0214. This star has rapid rotation, v sin (i)~ 40 km s-1, but generally shows no significant chromospheric emission. Our detection of the flare shows that a magnetic field is present …
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CITATION STYLE
APA
Reid, I. N., Kirkpatrick, J. D., Gizis, J. E., & Liebert, J. (1999). BRI 0021−0214: Another Surprise at the Bottom of the Main Sequence. The Astrophysical Journal, 527(2), L105–L107. https://doi.org/10.1086/312409
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