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[vsnet-obs 14762] Re: V3885 Sgr, this season
- Date: Mon, 07 Sep 1998 09:56:25 +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 14762] Re: V3885 Sgr, this season
- Disclaimer: The CSIR exercises no editorial control over E-mail messages originating in the organisation and the views in this message are therefore not necessarily those of the CSIR and/or its employees.
- Sender: owner-vsnet-obs@kusastro.kyoto-u.ac.jp
Hi,
V3885 Sgr is a novalike cv with high accretion flow. This makes it a
very blue object.
The shown visual estimates may be a point in case for the blue light
attenuation experienced in Japan, as pointed out by Dr T Kato or is
this a case of different sequences??
I used H/T!
Regards,
Berto
>>> Taichi Kato <tkato@kusastro.kyoto-u.ac.jp> 09/06 2:26 PM >>>
V3885 Sgr, this season
YYMMDD(UT) mag observer
980408.080 101 (B. Monard)
980419.930 103 (B. Monard)
980427.980 101 (B. Monard)
980502.149 102 (B. Monard)
980504.721 109 (T. Watanabe)
980522.694 109 (T. Watanabe)
980525.949 99 (B. Monard)
980530.698 109 (T. Watanabe)
980530.980 103 (B. Monard)
980619.860 101 (B. Monard)
980714.860 100 (B. Monard)
980727.780 100 (B. Monard)
980810.769 100 (B. Monard)
980813.780 99 (B. Monard)
980822.730 98 (B. Monard)
980823.542 109 (T. Watanabe)
980825.740 99 (B. Monard)
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