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[vsnet-obs 5278] VS observations by Ioh,Ino (T Pyx)
- Date: Thu, 13 Mar 1997 09:32:52 +0900 (JST)
- To: vsnet-obs
- From: Taichi Kato <tkato>
- Subject: [vsnet-obs 5278] VS observations by Ioh,Ino (T Pyx)
- Sender: owner-vsnet-obs@kusastro.kyoto-u.ac.jp
Visual magnitude estimates by VSOLJ members
object YYMMDD(UT) mag code
AURX 970312.597 90 Ioh.VSOLJ
CAMZ 970312.599 121 Ioh.VSOLJ
CETomicron 970311.419 37 Ioh.VSOLJ
CRBR 970312.613 60 Ioh.VSOLJ
GEMU 970311.522 <124 Ino.VSOLJ
LEOR 970311.546 84 Ino.VSOLJ
LEOT 970312.604 <136 Ioh.VSOLJ
LEOX 970311.550 <124 Ino.VSOLJ
MONU 970311.550 62 Ino.VSOLJ
PYXT 970311.536 <125 Ino.VSOLJ
PYXT 970311.625 130 Ino.VSOLJ (*1)
PYXT 970312.592 <106 Ioh.VSOLJ
Observer's code:
Ino: T.Inoue (Aichi,Japan) instruments: 40L,15R,8B
Ioh: H. Itoh (Tokyo, Japan) instruments: 30SC,5B
(*1) The observer reports "T Pyx visible by a 40-cm reflector (visual).
Also recorded by AVIS (I.I. + video), which clearly showed brightened
T Pyx at its proper location. Nearby 12.5 and 13.5 mag stars were clearly
identified." The observer used Burnham's handbook for identifying the
field.
While the observation still needs more independent confirmations,
there might have been a short brightness spike which might be somehow related
to the long-awaited forthcoming(?) eruption of this recurrent nova.