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[nova] PNV J145420000-5505030: Nova Lup 2011

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We performed optical spectroscopic observations (R about 400) of Nova Lup 2011 on 2011 Aug. 16.6 at Bosscha Observatory of Institut Teknologi Bandung using a 20-cm Schmidt-Cassegrain telescope with SBIG DSS7 spectrograph.  Our spectra exhibits strong H-alpha, H-beta and Fe II multiplet emissions, suggesting that the nova is a Fe-II type classical nova.  These results are consistent with previous reports in ATel #3536 and #3540.  P-Cygni profiles disappeared for any lines and the FWHM of the H-alpha emission is about 1700 km/s. This observation program is performed by the collaboration of Koyama Astronomical Obs. and Bosscha Obsrvatory, Institut Teknologi Bandung, Indonasia.

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