Hatena::Groupkanatatmp

KANATA ObsLog

2011-02-06

[] Nova Sgr 2011 : Observation start

f:id:kanataobslog:20110207041849p:image

We started the observations of nova Sgr 2011. This object is heavily reddened by interstellar dust. The raw V-J is 3.0, which is very red comparing with a typical value of classical nova in its peak. The V-band light curve shows the fast decline, which indicates that this nova would be classified into very fast nova, or still undergo in transitional phase. We continue the observations.