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[vsnet-alert 746] Re-brightening of T Leo
- Date: Sun, 23 Feb 1997 21:48:00 +0900 (JST)
- To: vsnet-alert
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsnet-alert 746] Re-brightening of T Leo
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
Observations to vsnet-obs indicate the dwarf nova T Leo is showing
a remarkable re-brightening, a presumable superoutburst triggered by the
'precursor' outburst on Feb. 19. Selected observations since the decline
of the first maximum:
YYMMDD(UT) mag code
970220.378 111 MRV
970220.447 111 MRV
970220.485 109 HSG
970220.624 107 Wnt
970220.717 11.25V Kis
970220.828 11.36V Kis
970221.198 118 MRV
970221.485 118 HSG
970221.708 <119 Wnt
970222.239 <129 HSG
970222.581 11.73V Kis
970222.635 <116 Wnt
970222.678 109 Ioh
970222.717 11.09V Kis
970223.180 108 MRV
970223.241 107 MRV
V-band CCD observations by S. Kiyota (vsnet-obs 5127) indicate superhumps
probably already appeared during the decline phase of the precursor outburst.
The present behavior strong resembles that observed during the initial stage
of the 1993 Jan. superoutburst (T. Kato, in preparation).
Regards,
Taichi Kato
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp