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[vsnet-alert 516] Re-brightening of Nova Sgr 1996
- Date: Mon, 19 Aug 1996 15:17:05 +0900
- To: nova@nova.la.asu.edu, vsnet-alert@sagano.kusastro.kyoto-u.ac.jp
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsnet-alert 516] Re-brightening of Nova Sgr 1996
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
Following observations reported to vsnet-obs seem to indicate Nova Sgr 1996
is undergoing a distinct re-brightening.
1996 Aug. 14.72 12.2 B. Monard
15.348 11.75V S. Kiyota (CCD, V-band)
16.748 12.0 B. Monard
16.892 11.8 B. Minard
17.547 11.71V D. Nogami, Ouda Station (CCD, V-band)
17.553 11.8 S. Takahashi
17.714 11.6 B. Monard
17.84 11.9 R. Fidrich
17.895 11.5 B. Monard
18.483 10.62V S. Kiyota (CCD, V-band)
Confirmation is strongly encouraged. Such large amplitude fluctuations
during the early post-maximum stage of novae were observed markedly in V443
Sct (Nova Sct 1989), and more recently in Nova Sgr 1994 No.2, the latter
accompanied by a subsequent deep dust minimum. Close monitoring of another
variety of recent series of "slow novae" would be interesting.
Regards,
Taichi Kato
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp