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).