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[nova] PNV J16364440-4132340

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We performed low-resolution optical spectroscopic observations of PN in Sco (cbat name is PNV J16364440-4132340) on 2011 Sep. 7.42 using the 1.3m Araki telescope with LOSA/F2 at Koyama Astronomical Observatory. The spectrum exhibits broad Balmer emission lines and Fe II multiplet emissions on a highly reddened continuum emission.  The H-alpha emission shows an assymmetric profile with FWZI about 6000 km/s.  Other significant features are invisible in our spectrum.  These results suggests that the object is an Fe II-type classical nova highly reddened by interstellar medium.

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2018/02

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