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[vsnet-alert 6498] V2275 Cyg spectrum by Fujii



V2275 Cyg spectrum by Fujii

    M. Fujii (Fujii Bisei Observatory) has further provided a spectrum
of V2275 Cyg (Nova Cyg 2001-2) taken on Aug. 22.50 UT.  The Balmer lines
have become more intensive compared to the spectrum taken on the first
night (Ayani, Bisei Observatory).  The FWHM of the H-alpha line is 3100 km/s.

    The spectrum can be seen at:
    http://vsnet1.harenet.ne.jp/~aikow/v2275_cyg.gif

    Based on the clear presence of Fe II multiplets, Fujii concluded that
the nova is a typical "Fe II-type" nova.

Relayed from M. Fujii

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