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[vsnet-obs 6075] Re: New Variables discovered by Tmz

   Thanks to Koyama-san to have forwarded these discovery reports by
K. Takamizawa during my absence.   I have changed the format somewhat
so that the data can become searchable by the VSNET data browser on the
Web.

TmzV06  940411.797  <150p  Tmz.VSOLJ
TmzV06  940506.684  <155p  Tmz.VSOLJ
TmzV06  940603.642  152p  Tmz.VSOLJ
TmzV06  940614.501  153p  Tmz.VSOLJ
TmzV06  940925.460  <150p  Tmz.VSOLJ
TmzV06  941022.385  <155p  Tmz.VSOLJ
TmzV06  950127.828  133p  Tmz.VSOLJ
TmzV06  950210.792  132p  Tmz.VSOLJ
TmzV06  950226.765  130p  Tmz.VSOLJ
TmzV06  950426.667  <155p  Tmz.VSOLJ
TmzV06  951013.406  151p  Tmz.VSOLJ
TmzV06  960126.828  <150p  Tmz.VSOLJ
TmzV06  960221.794  149p  Tmz.VSOLJ
TmzV06  960509.590  146p  Tmz.VSOLJ
TmzV06  960619.566  <155p  Tmz.VSOLJ
TmzV06  970212.810  <150p  Tmz.VSOLJ
TmzV06  970606.650  138p  Tmz.VSOLJ

   The variable TmzV06 has no IRAS PSC counterpart despite its large
amplitude (>2.5 mag) variation.  Checking the color on the current bright
occasion might be interesting.

TmzV07  940515.689  137p  Tmz.VSOLJ
TmzV07  940728.497  <145p  Tmz.VSOLJ
TmzV07  941102.392  <150p  Tmz.VSOLJ
TmzV07  941124.422  <150p  Tmz.VSOLJ
TmzV07  941219.363  <140p  Tmz.VSOLJ
TmzV07  950210.822  139p  Tmz.VSOLJ
TmzV07  950226.797  141p  Tmz.VSOLJ
TmzV07  950311.810  142p  Tmz.VSOLJ
TmzV07  950328.736  <140p  Tmz.VSOLJ
TmzV07  950419.767  143p  Tmz.VSOLJ
TmzV07  950423.658  145p  Tmz.VSOLJ
TmzV07  950522.697  <150p  Tmz.VSOLJ
TmzV07  950617.511  <140p  Tmz.VSOLJ
TmzV07  950619.567  <145p  Tmz.VSOLJ
TmzV07  950720.570  <140p  Tmz.VSOLJ
TmzV07  950804.635  <150p  Tmz.VSOLJ
TmzV07  950815.526  <140p  Tmz.VSOLJ
TmzV07  951014.460  <145p  Tmz.VSOLJ
TmzV07  951209.381  137p  Tmz.VSOLJ
TmzV07  960219.839  <140p  Tmz.VSOLJ
TmzV07  960721.555  <140p  Tmz.VSOLJ
TmzV07  961005.490  135p  Tmz.VSOLJ
TmzV07  961016.460  139p  Tmz.VSOLJ
TmzV07  961128.369  <145p  Tmz.VSOLJ
TmzV07  970308.801  <145p  Tmz.VSOLJ
TmzV07  970412.729  <145p  Tmz.VSOLJ
TmzV07  970613.610  121p  Tmz.VSOLJ

  The IRAS PSC counterpart of TmzV07 has a variablity probablity of 5%.
The data seem to suggest a Mira-type variable with a period near 280 d.

  Could anyone make follow-up observations of these new variables?

Regards,
Taichi Kato