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[vsnet-alert 4242] Nova Sgr 2000 brightening

Nova Sgr 2000 brightening

  Rod Stubbings and Andrew Pearce have reported that Nova Sgr 2000 has
brightened.  This may be a part of oscillations, as was observed in
Nova Sgr 1996, another Sakurai nova, in its early decline stage.

  YYYYMMDD(UT)   mag  observer
  20000125.863  115p  (Y. Sakurai)
  20000204.837  112p  (K. Takamizawa)
  20000204.842  112p  (K. Takamizawa)
  20000204.863  105p  (Y. Sakurai)
  20000206.812  104C  (Y. and R. Kushida (from IAUC))
  20000206.833  112p  (K. Haseda)
  20000206.837  112p  (K. Haseda)
  20000209.832  120p  (K. Takamizawa)
  20000209.842  120p  (K. Takamizawa)
  20000210.862  10.77C  (Ouda team)
  20000210.865  <104  (H. Maehara)
  20000211.503   123  (B. King)
  20000211.826   124  (T. Watanabe)
  20000211.837  109C  (Ageo Survey Team)
  20000211.848   124  (H. Maehara)
  20000212.713   122  (R. Stubbings)
  20000212.828   120  (A. Pearce)
  20000213.819   124  (A. Pearce)
  20000214.729   124  (R. Stubbings)
  20000214.837  9.84Ic  (S. Kiyota)
  20000214.841  12.11V  (S. Kiyota)
  20000214.844  13.63B  (S. Kiyota)
  20000214.853  10.85Rc  (S. Kiyota)
  20000215.732   127  (R. Stubbings)
  20000215.833  13.83B  (S. Kiyota)
  20000215.842  10.06Ic  (S. Kiyota)
  20000215.851  11.05Rc  (S. Kiyota)
  20000215.869  12.31V  (S. Kiyota)
  20000216.728   126  (R. Stubbings)
  20000216.815   128  (A. Pearce)
  20000217.747   121  (R. Stubbings)
  20000217.762   121  (R. Stubbings)
  20000217.826   124  (A. Pearce)

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