RECURRENT SYMBIOTIC NOVA V407 CYGNI: BEFORE AND AFTER OUTBURST IN 2010

被引：0

作者：

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

Kolotilov, E. A. ^{[1
]}

Shenavrin, V. I. ^{[1
]}

Tarasova, T. N. ^{[2
]}

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

Tatarnikova, A. A. ^{[1
]}

机构：

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

[2] Crimean Astrophys Observ, UA-298409 Nauchnyi, Crimea, Ukraine

来源：

BALTIC ASTRONOMY | 2015年 / 24卷 / 04期

基金：

俄罗斯基础研究基金会;

关键词：

binaries: symbiotic; stars: variables: Miras; stars: individual: V407 Cyg; RS-OPH; LITHIUM; VARIABILITY; PHOTOMETRY; STARS;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the results of our UBVJHKLM photometric and spectroscopic observations of V407 Cyg obtained in 2003-2015. No fast brightness variations of V407 Cyg have been detected since its RS Oph-type outburst in 2010. Now the binary demonstrates a low-excitation emission spectrum with Ha weaker than the [N II] 6584 angstrom line. It is a typical spectrum on the way to the passive state.

引用

页码：353 / 359

页数：7

共 50 条

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