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[vsnet-alert 1999] Apparent nova in M31
- Date: Tue, 4 Aug 1998 12:40:54 +0900 (JST)
- To: vsnet-alert, vsnet-chat
- From: Taichi Kato <tkato>
- Subject: [vsnet-alert 1999] Apparent nova in M31
- Cc: BMARSDEN@CFA.HARVARD.EDU, DGREEN@CFA.HARVARD.EDU
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
According to IAUC No. 6981, M. Modjaz et al. (KAIT team) discovered
an apparent nova in M31.
00h 42m 37s.00 (J2000.0)
+41o 16' 56".7
The reported unfiltered CCD magnitudes are
1998 Jul. 19.5 <18.0
23.5 16.1
27.5 14.4
31.5 15.6
Even considering the different CCD response to historical photographic
records, the peak brightness of 14.4 is remarkable. The brightest novae
ever discovered in M31 (disregarding SDOR stars and candidates) are:
max min maxJD name
M31V0748 NA 15.0 (18.6 2448244(1990) - - - ShA33
M31V0889 NA 15.0 (19.0 2445613(1983) - - - Nova1983
M31V0942 NA 15.0 (18. 2438707(1964) - - - Nova57
The record of other M31 (classical) novae seems to indicate the existence
of a sharp cut-off around 15.0 mag. Follow-up observations of the present
anomalously luminous (apparent) nova are thus highly recommended. Although
chance coincidence is very small, there may still exist a chance of a
foreground variable.
Historically, two novae were observed close to the location of the present
(apparent) nova. The difference in coordinates may safely preclude the
possibility of a recurrence.
004234.9 +411639 (2000.0) M31V0849 N 17.5 (19.0 24701(1926) - - - Nova64
004238.8 +411703 (2000.0) M31V0868 N 17.2 (18.5 22608(1920) - - - Nova18
Regards,
Taichi Kato
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