EARLY PHOTOMETRIC AND SPECTRAL EVOLUTION OF NOVA CYGNI 2014 (V2659 CYG)

被引：0

作者：

Burlak, M. A. ^{[1
]}

Esipov, V. F. ^{[1
]}

Komissarova, G. V. ^{[1
]}

机构：

[1] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Univ Skij Prospect 13, Moscow 119992, Russia

来源：

BALTIC ASTRONOMY | 2015年 / 24卷 / 04期

关键词：

novae; cataclysmic variables; stars: individual: V2659 Cyg;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present optical spectroscopic and UBV(RI)(C) photometric observations of Nova Cygni 2014 (V2659 Cyg) from its rebrightening to the nebular stage. After the first maximum, the nova underwent several irregular flare-like rebrightenings, with amplitudes up to two magnitudes, accompanied with spectral changes. During the bright state, forbidden lines became weaker; the absorption components of Balmer, He I, Fe II, N I, N II, O I lines strengthened, indicating an increase in the density and mass-loss rate in the form of a wind.

引用

页码：345 / 352

页数：8

共 16 条

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