文献
J-GLOBAL ID:202202259610312070
整理番号:22A1157418
単一中性子星の殻における非平衡化学組成形成の動的モデル【JST・京大機械翻訳】
Dynamic Model of a Non-equilibrium Chemical Composition Formation in the Shell of Single Neutron Stars
著者 (7件):
Ignatovskiy A. Yu.
(Space Research Institute, Russian Academy of Sciences, Moscow, Russia)
,
Ignatovskiy A. Yu.
(Moscow Institute of Physics and Technology, Moscow, Russia)
,
Ignatovskiy A. Yu.
(Institute for Theoretical and Experimental Physics of National Research Centr “Kurchatov Institute”, Moscow, Russia)
,
Ignatovskiy A. Yu.
(National Research Center “Kurchatov Institute”, Moscow, Russia)
,
Bisnovatyi-Kogan G. S.
(Space Research Institute, Russian Academy of Sciences, Moscow, Russia)
,
Bisnovatyi-Kogan G. S.
(Moscow Institute of Physics and Technology, Moscow, Russia)
,
Bisnovatyi-Kogan G. S.
(Moscow Engineering Physics Institute, Moscow, Russia)
資料名:
Astronomy Reports
(Astronomy Reports)
巻:
66
号:
3
ページ:
221-235
発行年:
2022年
JST資料番号:
W4072A
ISSN:
1063-7729
資料種別:
逐次刊行物 (A)
記事区分:
原著論文
発行国:
ドイツ (DEU)
言語:
英語 (EN)