THE SPECTRAL VARIATIONS OF VY MON IN 1986-1992

The variations of the 3-component profiles of the spectrum of VY Mon are reported which may be explained by restricted models of variable anisotropic stellar wind.

Bibliographic Details
Main Author: L. A. Pavlova
Format: Article
Language:English
Published: Odessa I. I. Mechnykov National University 2017-07-01
Series:Odessa Astronomical Publications
Online Access:http://oap.onu.edu.ua/article/view/105775
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spelling doaj-56df18589d2740dcad5e035c6663aa012020-11-25T02:59:58ZengOdessa I. I. Mechnykov National UniversityOdessa Astronomical Publications1810-42152017-07-017110.18524/1810-4215.1994.7.105775105775THE SPECTRAL VARIATIONS OF VY MON IN 1986-1992L. A. Pavlova0Fesenkov Astrophysical Institute, 480068 Almaty, KazakhstanThe variations of the 3-component profiles of the spectrum of VY Mon are reported which may be explained by restricted models of variable anisotropic stellar wind.http://oap.onu.edu.ua/article/view/105775
collection DOAJ
language English
format Article
sources DOAJ
author L. A. Pavlova
spellingShingle L. A. Pavlova
THE SPECTRAL VARIATIONS OF VY MON IN 1986-1992
Odessa Astronomical Publications
author_facet L. A. Pavlova
author_sort L. A. Pavlova
title THE SPECTRAL VARIATIONS OF VY MON IN 1986-1992
title_short THE SPECTRAL VARIATIONS OF VY MON IN 1986-1992
title_full THE SPECTRAL VARIATIONS OF VY MON IN 1986-1992
title_fullStr THE SPECTRAL VARIATIONS OF VY MON IN 1986-1992
title_full_unstemmed THE SPECTRAL VARIATIONS OF VY MON IN 1986-1992
title_sort spectral variations of vy mon in 1986-1992
publisher Odessa I. I. Mechnykov National University
series Odessa Astronomical Publications
issn 1810-4215
publishDate 2017-07-01
description The variations of the 3-component profiles of the spectrum of VY Mon are reported which may be explained by restricted models of variable anisotropic stellar wind.
url http://oap.onu.edu.ua/article/view/105775
work_keys_str_mv AT lapavlova thespectralvariationsofvymonin19861992
AT lapavlova spectralvariationsofvymonin19861992
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