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[vsnet-nl 21] MV Lyr rapid brightening

MV Lyr rapid brightening

   The VY Scl-type novalike variable MV Lyr has rapidly brightened.
The present brightening may have been dwarf nova-type, as judged from
the atypical speed of rise.  Time-series photometry is strongly encouraged
to clarify the present state (are superhumps visible?)

  YYYYMMDD(UT)   mag  observer
  20000820.149  <142  (M. Simonsen)
  20000821.014  <152  (G. Poyner)
  20000821.165  <142  (M. Simonsen)
  20000821.260  161V  (S. O'Connor)
  20000821.880  <140  (E. Muyllaert)
  20000822.149  <140  (M. Simonsen)
  20000822.855  <158  (M. Reszelski)
  20000822.873  <140  (E. Muyllaert)
  20000822.949  <152  (G. Poyner)
  20000823.867  <140  (E. Muyllaert)
  20000823.915   159: (M. Reszelski)
  20000824.925  <140  (E. Muyllaert)
  20000825.008  <152  (G. Poyner)
  20000825.140  <140  (M. Simonsen)
  20000825.844   160: (M. Reszelski)
  20000825.864  <140  (E. Muyllaert)
  20000826.853  <140  (E. Muyllaert)
  20000826.860  <157  (M. Reszelski)
  20000826.942  <152  (G. Poyner)
  20000827.572  <131  (H. Maehara)
  20000827.853  <140  (E. Muyllaert)
  20000828.856  <140  (E. Muyllaert)
  20000828.931   142  (G. Poyner)
  20000829.040   137  (M. Verdenet)
  20000829.840   139  (M. Reszelski)
  20000829.856   140  (E. Muyllaert)
  20000831.130   140  (M. Simonsen)
  20000831.256   142  (G. Hanson)

Regards,
Taichi Kato
VSNET Collaboration team

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