VV Pup
The VSNET administrator team received a request from FUSE team to
ask VSNET team to observe VV Pup (polar) on April 5 and 6, in order to
know the current activity state during the FUSE observation. This
system has a 100 min orbital period and a large hump when the pole is
in view if it is in an active state
(vsnet-campaign 838).
The Kyoto team performed an observation on April 5
(vsnet-campaign 839).
The analysis of the Kyoto optical observation (by Ishioka-san),
quasi-simultaneous with the FUSE observation, showed sharp and giant
hump (15.24 - 17.7 mag). This observation indicate that VV Pup
was in actively accreting state at least during this run
(vsnet-campaign 844,
845,
846).
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vsnet-adm@kusastro.kyoto-u.ac.jp
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