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[vsnet-newvar 1642] (fwd) Position of Liller's nova suspect in SMC
- Date: Sat, 19 Oct 2002 13:45:52 +0900 (JST)
- To: vsnet-campaign-nova@ooruri.kusastro.kyoto-u.ac.jp, vsnet-discovery-nova@ooruri.kusastro.kyoto-u.ac.jp
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsnet-newvar 1642] (fwd) Position of Liller's nova suspect in SMC
- Cc: vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp
(fwd) Position of Liller's nova suspect in SMC
I note that Bill Liller's nova suspect in the SMC is virtually coincident
with a USNO-A2.0 star (r=16.2, b=17.7, V= 16.8) at 0h56m30.26s -726'29.4".
This star is shown on Fig. 4 of the paper by J. Vigneau and M. Azzopardi
(1982), having two close companions to the SW. These authors also provide a
UBVRI sequence ("Sequence II") for this field. The "nova" falls exactly on
the line between their stars #1 and #7, and 45.5mm from star 1.
A better position for the "nova" is essential to resolve this matter.
Ref.
Vigneau, J., Azzopardi, M. 1982. Astron. Astrophys. Suppl. 50, 119-127.
Regards,
Mati
morel@ozemail.com.au
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