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
C. Lloyd commented that Brh V84 is more likely to be a dMe (or similar)
than an algol
T. Kato however mentioned that the X-ray spectrum of this object is
harder than most of dMe stars