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[vsnet-chat 777] Re: [vsnet-obs 10644] CCD observations by Kis (Nova Sgr, TUCrt)
- Date: Thu, 26 Mar 1998 09:12:04 +0200
- To: tkato@kusastro.kyoto-u.ac.jp, vsnet-chat@kusastro.kyoto-u.ac.jp
- From: Berto Monard <lagmonar@csir.co.za>
- Subject: [vsnet-chat 777] Re: [vsnet-obs 10644] CCD observations by Kis (Nova Sgr, TUCrt)
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- Encoding: 27 Text
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Dear readers,
The hot accretion disc in a nova event is supposed to shine at blue-UV-X wavelengths.
The CCD measures from Seiichiro Kiyota show the nova 'wears' red... Any comments?
Perhaps some strong emission lines coincide with the V and R wavelength fields?
Berto Monard
>>> Taichi Kato <tkato@kusastro.kyoto-u.ac.jp> 03/26 4:23 AM >>>
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PHOTOMETRIC CCD OBSERVATIONS OF VARIABLE STARS
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CENTER FOR BALCONY ASTROPHYSICS (CBA) Tsukuba, JAPAN
Observer: Seiichiro Kiyota
E-mail: skiyota@abr.affrc.go.jp
WWW: http://vsnet.age.ne.jp/x/meineko/index-e.html
Instruments: 0.25-m + Bitran BT-20 + Optec Maxfilter 2"
object YYMMDD(UT) mag code
CRTTU 980325.722 128: Kis.VSOLJ
SGRnova1998 980325.747 7.92V Kis.VSOLJ seq: HIP 8.10
SGRnova1998 980325.757 8.42B Kis.VSOLJ
SGRnova1998 980325.767 7.40Rc Kis.VSOLJ
!
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