Hatena::Groupkanatatmp

KANATA ObsLog

2011-05-14

[] V5588 Sgr : rebrightening and decline

f:id:kanataobslog:20110515035536p:image

We performed the optical and near-infrared photometry of V5588 Sgr. The light curves in all-bands exhibit the rebrightening at around 30 days after discovery. We find that the ejected material did not pronouncedly form the dust.