Standard

Emission from an inhomogeneous plasma : Line intensities and determination of elemental abundances in gaseous nebulae with fluctuations of Te and ne. / Kholtygin, A. F.

в: Astrophysics, Том 43, № 4, 01.01.2000, стр. 463-473.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Kholtygin, AF 2000, 'Emission from an inhomogeneous plasma: Line intensities and determination of elemental abundances in gaseous nebulae with fluctuations of Te and ne', Astrophysics, Том. 43, № 4, стр. 463-473. https://doi.org/10.1023/A:1010975110093

APA

Kholtygin, A. F. (2000). Emission from an inhomogeneous plasma: Line intensities and determination of elemental abundances in gaseous nebulae with fluctuations of Te and ne. Astrophysics, 43(4), 463-473. https://doi.org/10.1023/A:1010975110093

Vancouver

Kholtygin AF. Emission from an inhomogeneous plasma: Line intensities and determination of elemental abundances in gaseous nebulae with fluctuations of Te and ne. Astrophysics. 2000 Янв. 1;43(4):463-473. https://doi.org/10.1023/A:1010975110093

Author

Kholtygin, A. F. / Emission from an inhomogeneous plasma : Line intensities and determination of elemental abundances in gaseous nebulae with fluctuations of Te and ne. в: Astrophysics. 2000 ; Том 43, № 4. стр. 463-473.

BibTeX

@article{20e47653c45745bfa2765f80f03402e8,
title = "Emission from an inhomogeneous plasma: Line intensities and determination of elemental abundances in gaseous nebulae with fluctuations of Te and ne",
abstract = "A method is proposed for determining the abundances of chemical elements in planetary nebulae based on allowance for the actual distribution functions of errors in measuring line intensities. Fluctuations both in temperature and in mass density of a nebula are taken into account in the proposed method. The results of a determination of C and O abundances and of the amplitudes of temperature and density fluctuations are given.",
author = "Kholtygin, {A. F.}",
year = "2000",
month = jan,
day = "1",
doi = "10.1023/A:1010975110093",
language = "English",
volume = "43",
pages = "463--473",
journal = "Astrophysics",
issn = "0571-7256",
publisher = "Wolters Kluwer",
number = "4",

}

RIS

TY - JOUR

T1 - Emission from an inhomogeneous plasma

T2 - Line intensities and determination of elemental abundances in gaseous nebulae with fluctuations of Te and ne

AU - Kholtygin, A. F.

PY - 2000/1/1

Y1 - 2000/1/1

N2 - A method is proposed for determining the abundances of chemical elements in planetary nebulae based on allowance for the actual distribution functions of errors in measuring line intensities. Fluctuations both in temperature and in mass density of a nebula are taken into account in the proposed method. The results of a determination of C and O abundances and of the amplitudes of temperature and density fluctuations are given.

AB - A method is proposed for determining the abundances of chemical elements in planetary nebulae based on allowance for the actual distribution functions of errors in measuring line intensities. Fluctuations both in temperature and in mass density of a nebula are taken into account in the proposed method. The results of a determination of C and O abundances and of the amplitudes of temperature and density fluctuations are given.

UR - http://www.scopus.com/inward/record.url?scp=42449120857&partnerID=8YFLogxK

U2 - 10.1023/A:1010975110093

DO - 10.1023/A:1010975110093

M3 - Article

AN - SCOPUS:42449120857

VL - 43

SP - 463

EP - 473

JO - Astrophysics

JF - Astrophysics

SN - 0571-7256

IS - 4

ER -

ID: 36162956