[nova] PNV J16364440-4132340
- 2011/09/08 00:50
- posted by: 新井彰(ARAI, Akira)
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.