Standard

Chemical evolution of the system of galactic planetary nebulae. / Lunyova, Yu V.; Kholtygin, A. F.

In: Astrophysics, Vol. 45, No. 3, 01.01.2002, p. 370-379.

Research output: Contribution to journal › Article › peer-review

Harvard

Lunyova, YV & Kholtygin, AF 2002, 'Chemical evolution of the system of galactic planetary nebulae', Astrophysics, vol. 45, no. 3, pp. 370-379. https://doi.org/10.1023/A:1020151919593

APA

Lunyova, Y. V., & Kholtygin, A. F. (2002). Chemical evolution of the system of galactic planetary nebulae. Astrophysics, 45(3), 370-379. https://doi.org/10.1023/A:1020151919593

Vancouver

Lunyova YV, Kholtygin AF. Chemical evolution of the system of galactic planetary nebulae. Astrophysics. 2002 Jan 1;45(3):370-379. https://doi.org/10.1023/A:1020151919593

Author

Lunyova, Yu V. ; Kholtygin, A. F. / Chemical evolution of the system of galactic planetary nebulae. In: Astrophysics. 2002 ; Vol. 45, No. 3. pp. 370-379.

BibTeX

@article{892ae4b8d99c49b08ef88b31d943672f,
title = "Chemical evolution of the system of galactic planetary nebulae",
abstract = "The problem of the chemical evolution of the system of Galactic planetary nebulae, starting with the early stage of development of the Galaxy, is investigated. The radial and vertical gradients of C, N, O, Ne, Ar, Cl, and S abundances are determined for different ages of the precursor stars of the nebulae. A statistically significant age dependence of the gradients is derived.",
keywords = "Abundances, Evolution, Planetary nebulae",
author = "Lunyova, {Yu V.} and Kholtygin, {A. F.}",
year = "2002",
month = jan,
day = "1",
doi = "10.1023/A:1020151919593",
language = "English",
volume = "45",
pages = "370--379",
journal = "Astrophysics",
issn = "0571-7256",
publisher = "Wolters Kluwer",
number = "3",

}

RIS

TY - JOUR

T1 - Chemical evolution of the system of galactic planetary nebulae

AU - Lunyova, Yu V.

AU - Kholtygin, A. F.

PY - 2002/1/1

Y1 - 2002/1/1

N2 - The problem of the chemical evolution of the system of Galactic planetary nebulae, starting with the early stage of development of the Galaxy, is investigated. The radial and vertical gradients of C, N, O, Ne, Ar, Cl, and S abundances are determined for different ages of the precursor stars of the nebulae. A statistically significant age dependence of the gradients is derived.

AB - The problem of the chemical evolution of the system of Galactic planetary nebulae, starting with the early stage of development of the Galaxy, is investigated. The radial and vertical gradients of C, N, O, Ne, Ar, Cl, and S abundances are determined for different ages of the precursor stars of the nebulae. A statistically significant age dependence of the gradients is derived.

KW - Abundances

KW - Evolution

KW - Planetary nebulae

UR - http://www.scopus.com/inward/record.url?scp=2142673807&partnerID=8YFLogxK

U2 - 10.1023/A:1020151919593

DO - 10.1023/A:1020151919593

M3 - Article

AN - SCOPUS:2142673807

VL - 45

SP - 370

EP - 379

JO - Astrophysics

JF - Astrophysics

SN - 0571-7256

IS - 3

ER -

ID: 36162701