18 Jul
2023
18 Jul
'23
9:02 a.m.
V2276 Sgr: oscillation-type rebrightening
Josch Hambsch reported further observations. The object is now in an oscillation state, commonly seen in AM CVn-type superoutburst. I obtained a likely period of 0.02019 d, which also appears suitable for an AM CVn star, but requires confirmation since observations are still lacking.