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[Possible Nova in M31] PNV J00414112+4120117

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We performed low-dispersion optical spectroscopic observations of Possible Nova in M31 (= PNV J00414112+4120117) using the 1.3m Araki telescope on 2011 August 03.7UT.

The red spectrum in the figure shows our preliminary spectrum of PNV J00414112+4120117. Our spectra of PNV J00424483+4118007 and V5588 Sgr are also shown. 

The spectrum exhibits the broad H-alpha, H-beta emissions (FWHM about 1600 km/s) and Fe II multiplet emission features, which suggest that the object is a Fe II-type classical nova after the maximum.

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