Brh V84 : Erruptive variable?

Brh V84 is identified with a ROSAT source. This field has been surveyed by MSX5C, but has no bright infrared counterpart, making the identification as an SR or long-period variable unlikely. Although the object may be an active Algol, this variable apparently warrants further detailed study, including spectroscopy (vsnet-campaign 1006). C. Lloyd commented that Brh V84 is more likely to be a dMe (or similar) than an algol (vsnet-campaign 1007). T. Kato however mentioned that the X-ray spectrum of this object is harder than most of dMe stars (vsnet-campaign 1008).

Light Curve of This Object