Super-Alfvén Expansion of a Nova Shell in the Magnetic Field of Its Core Full article
Journal |
Astronomy Letters
ISSN: 1063-7737 , E-ISSN: 1562-6873 |
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Output data | Year: 2000, Volume: 26, Number: 6, Pages: 362-371 Pages count : 10 DOI: 10.1134/1.20403 | ||||||
Tags | Hydrodynamics and shock waves, Plasma astrophysics | ||||||
Authors |
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Affiliations |
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Funding (1)
1 | Russian Foundation for Basic Research | 97-02-18471 |
Abstract:
We study the effect of nova magnetodipole fields on the dynamics and structure of ejected shells by using a numerical model based on the kinetic-hydrodynamic description of plasma dynamics. Our calculations show that characteristic nonuniformities appear in the distribution of field and plasma perturbations during super-Alfvén shell expansion in the circumstellar medium.
Cite:
Nikitin S.A.
, Vshivkov V.A.
, Snytnikov V.N.
Super-Alfvén Expansion of a Nova Shell in the Magnetic Field of Its Core
Astronomy Letters. 2000. V.26. N6. P.362-371. DOI: 10.1134/1.20403 WOS Scopus РИНЦ
Super-Alfvén Expansion of a Nova Shell in the Magnetic Field of Its Core
Astronomy Letters. 2000. V.26. N6. P.362-371. DOI: 10.1134/1.20403 WOS Scopus РИНЦ
ArticleLinkType.TRANSLATED_TO_ORIGINAL:
Никитин С.А.
, Вшивков В.А.
, Снытников В.Н.
Сверхальвеновское расширение оболочки новой звезды в магнитном поле ее ядра
Письма в Астрономический журнал: Астрономия и космическая астрофизика. 2000. Т.26. №6. С.427-436. РИНЦ
Сверхальвеновское расширение оболочки новой звезды в магнитном поле ее ядра
Письма в Астрономический журнал: Астрономия и космическая астрофизика. 2000. Т.26. №6. С.427-436. РИНЦ
Dates:
Submitted: | Apr 13, 1999 |
Published print: | Jun 1, 2000 |
Identifiers:
Web of science | WOS:000088034700004 |
Scopus | 2-s2.0-0034393528 |
Elibrary | 13340638 |
OpenAlex | W1981672386 |