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[vsnet-alert 806] outburst of OY Car
- Date: Thu, 27 Mar 1997 14:45:59 +0900 (JST)
- To: vsnet-alert
- From: Taichi Kato <tkato>
- Subject: [vsnet-alert 806] outburst of OY Car
- Cc: mauche@cygnus.llnl.gov
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
Following the initial alert by Michael Mattiazzo (vsnet-alert 802),
following observations have been reported to vsnet-alert and vsnet-obs.
YYMMDD(UT) mag code
970312.497 <127 MKA
970316.433 <127 MKA
970325.424 117 MKA
970325.453 116 MKA
970325.562 116 MKA
970326.417 114 MKA
970326.458 115 MKA
970326.500 116 MKA
970326.542 115 MKA
970326.801 111 HJN
Judging from the brightness and duration, the present outburst may well
be a superoutburst, since its last one in 1995 October - November.
OY Car is one of the most well-known eclipsing SU UMa-type dwarf novae,
which have been and will be teaching us much about the physical processes
going in superoutbursting dwarf novae. OY Car has played an important
role in this field [1,2,3].
[1] J. H. Wood et al., 1989, ApJ 341, 974
[2] F. V. Hessman et al., 1992, AsAp 263, 147
(OY Carinae: the secrets of the super-humps revealed)
[3] I. Billington et al., 1996, MNRAS, 279, 1274 and references therein
I would also like to urge visual (and CCD, of course) observers to record
spectacular eclipses (together with possible superhumps) of this short-period
cataclysmic binary. A good northern example may be found at
(http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/htcas.html).
According to [1], eclipse are expected to occur:
HJED = 2443993.553691 + 0.0631209295 E
+/-50 +/-20
Regards,
Taichi Kato
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vsnet-adm@kusastro.kyoto-u.ac.jp