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[vsnet-alert 4725] Re: CI Aql = recurrent Nova Aql 2000
- Date: Sun, 30 Apr 2000 17:10:55 +0900 (JST)
- To: vsnet-alert@kusastro.kyoto-u.ac.jp
- From: Hitoshi YAMAOKA <yamaoka@rc.kyushu-u.ac.jp>
- Subject: [vsnet-alert 4725] Re: CI Aql = recurrent Nova Aql 2000
- Cc: ayani@bao.go.jp, yamaoka@rcsvr.rc.kyushu-u.ac.jp, meineko@x.age.ne.jp
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
Dear all,
With Bisei image, I could get more accurate position of probable
nova in Aquila = the recurrence of CI Aql (Nova Aql 1917). I reported
to CBAT as below.
----
PROBABLE NOVA IN AQUILA = the recurrence of CI Aql
H. Yamaoka, Kyushu University, reports the accurate position of
the probable nova in Aquila (IAUC 7409), measured with the
unfiltered CCD image taken with Bisei 1.01-m telescope by K. Ayani,
Bisei Astronomical Observatory, and K. Shirakami, Okayama, Japan, as
R.A. = 18h52m03s.55, Decl. = -01o28'38".9 (equinox 2000.0,
uncertainty around 0".2). This position is nearly identical to that
of the eclipsing binary, which was proposed to be the quiescent
counterpart of the suspected nova 1917 (IBVS 4338 and Duerbeck 1987,
SSR, 45, 1). It is strongly suggested that the suspected Nova Aql
1917 = CI Aql was real and the ongoing eruption is the recurrence of
it.
Sincerely Yours,
Hitoshi Yamaoka, Kyushu Univ., Japan
yamaoka@rc.kyushu-u.ac.jp
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp