Electronic Telegram No. 4333
Central Bureau for Astronomical Telegrams
Mailing address:  Hoffman Lab 209; Harvard University;
 20 Oxford St.; Cambridge, MA  02138; U.S.A.
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Prepared using the Tamkin Foundation Computer Network


NOVA IN SAGITTARIUS = TCP J18102829-2729590
     K. Ayani, Bisei Astronomical Observatory (BAO), Ibara, Okayama, obtained
a low-resolution spectrogram (range 400-800 nm; resolution 0.5 nm at H-alpha)
of TCP J18102829-2729590 (cf. CBET 4332) with the BAO 1.01-m telescope on Oct.
24.38 UT.  The spectrum shows absorption lines of Balmer lines, Fe II (42),
Na D, and O I 777.4-nm.  The H-alpha and O I lines show P-Cyg profiles.  The
absorption bottom of H-alpha is blueshifted by 600 km/s with respect to the
emission peak.  This confirms that the object is a nova in early phase.  The
spectrum is viewable via website URL http://tinyurl.com/z6pqe3v.


NOTE: These 'Central Bureau Electronic Telegrams' are sometimes
      superseded by text appearing later in the printed IAU Circulars.

                         (C) Copyright 2016 CBAT
2016 October 25                  (CBET 4333)              Daniel W. E. Green