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[vsnet-obs 10671] Re: Outburst of TU Crt (update)
- Date: Thu, 26 Mar 1998 10:49:23 +0200
- To: tkato@kusastro.kyoto-u.ac.jp, vsnet-obs@kusastro.kyoto-u.ac.jp
- From: Berto Monard <lagmonar@csir.co.za>
- Subject: [vsnet-obs 10671] Re: Outburst of TU Crt (update)
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- Sender: owner-vsnet-obs@kusastro.kyoto-u.ac.jp
To whom it may..
there are no official relevant sequences (at least not known to me and some others to whom I discussed it) for the TU Crt region. The scatter in observed magnitudes is a direct result.
I did however anchor my observations to the brightness of one (one only and yes, that's not good enough...) of the nearby stars.
At any time I could therefore modify my results to fall in line with wathever sequences will be endorsed in the future.
Regards,
Berto Monard
>>> Taichi Kato <tkato@kusastro.kyoto-u.ac.jp> 03/26 10:08 AM >>>
Outburst of TU Crt (update)
Still bright!
YYMMDD(UT) mag observer
980322.469 <150 (R. Stubbings)
980323.290 <137 (B. Monard)
980323.750 <137 (B. Monard)
980323.890 <130 (P. Schmeer)
980324.449 150 (R. Stubbings)
980324.476 145 (R. Stubbings)
980324.502 139 (R. Stubbings)
980324.522 136 (R. Stubbings)
980324.595 130 (R. Stubbings)
980324.680 128 (R. Stubbings)
980324.781 124 (B. Monard)
980324.828 124 (B. Monard)
980324.908 127 (P. Schmeer)
980324.916 124 (B. Monard)
980325.449 123 (R. Stubbings)
980325.722 128: (S. Kiyota)
980325.750 124 (B. Monard)
!
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