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2005IAUC.8506....3Y - IAU Circ., 8506, 3 (2005/April-0)
V378 Serpentis = possible nova in Serpens.
YAMAOKA H. and FUJII M.
Abstract (from CDS):
H. Yamaoka, Kyushu University, communicates that M. Fujii (Okayama, Japan) obtained a spectrogram of this nova on Apr. 4.80 UT with a 0.28-m telescope. The spectrum shows strong and broad Balmer emission lines (FWHM = 1100 km/s for H_alpha) with P-Cyg profile and several Fe II and O I 777.3-nm emission lines, which suggests that it is a Fe II-class nova somewhat after maximum light.
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Simbad objects: 1
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