THE MASSES OF THE IONIZED GAS OF PLANETARY NEBULAE ENVELOPES IN LARGE MAGELLANIC CLOUD

The masses of ionized gas in the shells of planetary nebulae which belong in the Large Magellanic Cloud are calculated by three different ways. The value of mass is calculated for the cases: 1) spherical, 2) elliptical forms of envelopes and 3) commonly known method based on the line ratio F(Hβ) of...

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Main Authors: V. Holovatyy, A. Demchyna
Format: Article
Language:English
Published: Odessa I. I. Mechnykov National University 2013-11-01
Series:Odessa Astronomical Publications
Subjects:
Online Access:http://oap.onu.edu.ua/article/view/81829
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author V. Holovatyy
A. Demchyna
author_facet V. Holovatyy
A. Demchyna
author_sort V. Holovatyy
collection DOAJ
description The masses of ionized gas in the shells of planetary nebulae which belong in the Large Magellanic Cloud are calculated by three different ways. The value of mass is calculated for the cases: 1) spherical, 2) elliptical forms of envelopes and 3) commonly known method based on the line ratio F(Hβ) of the shell to its emissivity of  ε(Hβ). It is shown that the values of masses Mi  of nebulae envelopes differ up to 50%. The values of  Mi  calculated by the other methods which differ more from previous ones. We consider the dependence of Mi  on the radius and the electron density in the envelopes of nebulae.
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spelling doaj.art-19dc1cb39bbd44c4bf8562e64120d8f12022-12-21T23:47:25ZengOdessa I. I. Mechnykov National UniversityOdessa Astronomical Publications1810-42152013-11-01261616210.18524/1810-4215.2013.26.8182981829THE MASSES OF THE IONIZED GAS OF PLANETARY NEBULAE ENVELOPES IN LARGE MAGELLANIC CLOUDV. Holovatyy0A. Demchyna1Ivan Franko National University of LvivIvan Franko National University of LvivThe masses of ionized gas in the shells of planetary nebulae which belong in the Large Magellanic Cloud are calculated by three different ways. The value of mass is calculated for the cases: 1) spherical, 2) elliptical forms of envelopes and 3) commonly known method based on the line ratio F(Hβ) of the shell to its emissivity of  ε(Hβ). It is shown that the values of masses Mi  of nebulae envelopes differ up to 50%. The values of  Mi  calculated by the other methods which differ more from previous ones. We consider the dependence of Mi  on the radius and the electron density in the envelopes of nebulae.http://oap.onu.edu.ua/article/view/81829mass of ionized gasplanetary nebulae of lmc
spellingShingle V. Holovatyy
A. Demchyna
THE MASSES OF THE IONIZED GAS OF PLANETARY NEBULAE ENVELOPES IN LARGE MAGELLANIC CLOUD
Odessa Astronomical Publications
mass of ionized gas
planetary nebulae of lmc
title THE MASSES OF THE IONIZED GAS OF PLANETARY NEBULAE ENVELOPES IN LARGE MAGELLANIC CLOUD
title_full THE MASSES OF THE IONIZED GAS OF PLANETARY NEBULAE ENVELOPES IN LARGE MAGELLANIC CLOUD
title_fullStr THE MASSES OF THE IONIZED GAS OF PLANETARY NEBULAE ENVELOPES IN LARGE MAGELLANIC CLOUD
title_full_unstemmed THE MASSES OF THE IONIZED GAS OF PLANETARY NEBULAE ENVELOPES IN LARGE MAGELLANIC CLOUD
title_short THE MASSES OF THE IONIZED GAS OF PLANETARY NEBULAE ENVELOPES IN LARGE MAGELLANIC CLOUD
title_sort masses of the ionized gas of planetary nebulae envelopes in large magellanic cloud
topic mass of ionized gas
planetary nebulae of lmc
url http://oap.onu.edu.ua/article/view/81829
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