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On mass simulations of dynamical models of galaxy. / Davydenko, Alexander A.; Raspopova, Natalya V.; Ustimenko, Sergei S.

2015 International Conference on "Stability and Control Processes" in Memory of V.I. Zubov, SCP 2015 - Proceedings. ред. / L. A. Petrosyan; A. P. Zhabko. Institute of Electrical and Electronics Engineers Inc., 2015. стр. 42-44 7342053 (2015 International Conference on "Stability and Control Processes" in Memory of V.I. Zubov, SCP 2015 - Proceedings).

Результаты исследований: Публикации в книгах, отчётах, сборниках, трудах конференцийстатья в сборнике материалов конференциинаучнаяРецензирование

Harvard

Davydenko, AA, Raspopova, NV & Ustimenko, SS 2015, On mass simulations of dynamical models of galaxy. в LA Petrosyan & AP Zhabko (ред.), 2015 International Conference on "Stability and Control Processes" in Memory of V.I. Zubov, SCP 2015 - Proceedings., 7342053, 2015 International Conference on "Stability and Control Processes" in Memory of V.I. Zubov, SCP 2015 - Proceedings, Institute of Electrical and Electronics Engineers Inc., стр. 42-44, III Международная конференция "Устойчивость и процессы управления", посвященная 85-летию со дня рождения чл.-корр. РАН В.И. Зубова, St. Petersburg, Российская Федерация, 5/10/15. https://doi.org/10.1109/SCP.2015.7342053, https://doi.org/10.1109/SCP.2015.7342053

APA

Davydenko, A. A., Raspopova, N. V., & Ustimenko, S. S. (2015). On mass simulations of dynamical models of galaxy. в L. A. Petrosyan, & A. P. Zhabko (Ред.), 2015 International Conference on "Stability and Control Processes" in Memory of V.I. Zubov, SCP 2015 - Proceedings (стр. 42-44). [7342053] (2015 International Conference on "Stability and Control Processes" in Memory of V.I. Zubov, SCP 2015 - Proceedings). Institute of Electrical and Electronics Engineers Inc.. https://doi.org/10.1109/SCP.2015.7342053, https://doi.org/10.1109/SCP.2015.7342053

Vancouver

Davydenko AA, Raspopova NV, Ustimenko SS. On mass simulations of dynamical models of galaxy. в Petrosyan LA, Zhabko AP, Редакторы, 2015 International Conference on "Stability and Control Processes" in Memory of V.I. Zubov, SCP 2015 - Proceedings. Institute of Electrical and Electronics Engineers Inc. 2015. стр. 42-44. 7342053. (2015 International Conference on "Stability and Control Processes" in Memory of V.I. Zubov, SCP 2015 - Proceedings). https://doi.org/10.1109/SCP.2015.7342053, https://doi.org/10.1109/SCP.2015.7342053

Author

Davydenko, Alexander A. ; Raspopova, Natalya V. ; Ustimenko, Sergei S. / On mass simulations of dynamical models of galaxy. 2015 International Conference on "Stability and Control Processes" in Memory of V.I. Zubov, SCP 2015 - Proceedings. Редактор / L. A. Petrosyan ; A. P. Zhabko. Institute of Electrical and Electronics Engineers Inc., 2015. стр. 42-44 (2015 International Conference on "Stability and Control Processes" in Memory of V.I. Zubov, SCP 2015 - Proceedings).

BibTeX

@inproceedings{496202cb430841f8bb482190c6460007,
title = "On mass simulations of dynamical models of galaxy",
abstract = "In the present paper we consider spherically and axially symmetric stellar system models in order to examine the character of orbits of stars moving in the gravitational field. We study orbits in the meridian plane for the model with the massive nucleus varying values of the structural parameters, as well as two integrals of motion. In an attempt to distinguish regular and chaotic motions we use surfaces of section. We numerically investigate the orbits of star cluster moving in the plane of the galaxy in a circular orbit. The impact of initial conditions on the star movements and probability to escape from the cluster are examined. Calculations of star orbits for various initial values of energy and momentum has been done. Simulations showed that retrograde orbits of stars are more stable than regular ones.",
keywords = "Computational modeling, Electronic mail, Mathematical model, Numerical models, Orbits, Structural engineering, Trajectory",
author = "Davydenko, {Alexander A.} and Raspopova, {Natalya V.} and Ustimenko, {Sergei S.}",
note = "Publisher Copyright: {\textcopyright} 2015 IEEE. Copyright: Copyright 2017 Elsevier B.V., All rights reserved.; International Conference on {"}Stability and Control Processes{"} in Memory of V.I. Zubov, SCP 2015 ; Conference date: 05-10-2015 Through 09-10-2015",
year = "2015",
month = nov,
day = "30",
doi = "10.1109/SCP.2015.7342053",
language = "English",
series = "2015 International Conference on {"}Stability and Control Processes{"} in Memory of V.I. Zubov, SCP 2015 - Proceedings",
publisher = "Institute of Electrical and Electronics Engineers Inc.",
pages = "42--44",
editor = "Petrosyan, {L. A.} and Zhabko, {A. P.}",
booktitle = "2015 International Conference on {"}Stability and Control Processes{"} in Memory of V.I. Zubov, SCP 2015 - Proceedings",
address = "United States",
url = "http://www.apmath.spbu.ru/scp2015/openconf.php",

}

RIS

TY - GEN

T1 - On mass simulations of dynamical models of galaxy

AU - Davydenko, Alexander A.

AU - Raspopova, Natalya V.

AU - Ustimenko, Sergei S.

N1 - Publisher Copyright: © 2015 IEEE. Copyright: Copyright 2017 Elsevier B.V., All rights reserved.

PY - 2015/11/30

Y1 - 2015/11/30

N2 - In the present paper we consider spherically and axially symmetric stellar system models in order to examine the character of orbits of stars moving in the gravitational field. We study orbits in the meridian plane for the model with the massive nucleus varying values of the structural parameters, as well as two integrals of motion. In an attempt to distinguish regular and chaotic motions we use surfaces of section. We numerically investigate the orbits of star cluster moving in the plane of the galaxy in a circular orbit. The impact of initial conditions on the star movements and probability to escape from the cluster are examined. Calculations of star orbits for various initial values of energy and momentum has been done. Simulations showed that retrograde orbits of stars are more stable than regular ones.

AB - In the present paper we consider spherically and axially symmetric stellar system models in order to examine the character of orbits of stars moving in the gravitational field. We study orbits in the meridian plane for the model with the massive nucleus varying values of the structural parameters, as well as two integrals of motion. In an attempt to distinguish regular and chaotic motions we use surfaces of section. We numerically investigate the orbits of star cluster moving in the plane of the galaxy in a circular orbit. The impact of initial conditions on the star movements and probability to escape from the cluster are examined. Calculations of star orbits for various initial values of energy and momentum has been done. Simulations showed that retrograde orbits of stars are more stable than regular ones.

KW - Computational modeling

KW - Electronic mail

KW - Mathematical model

KW - Numerical models

KW - Orbits

KW - Structural engineering

KW - Trajectory

UR - http://www.scopus.com/inward/record.url?scp=84960104442&partnerID=8YFLogxK

U2 - 10.1109/SCP.2015.7342053

DO - 10.1109/SCP.2015.7342053

M3 - Conference contribution

T3 - 2015 International Conference on "Stability and Control Processes" in Memory of V.I. Zubov, SCP 2015 - Proceedings

SP - 42

EP - 44

BT - 2015 International Conference on "Stability and Control Processes" in Memory of V.I. Zubov, SCP 2015 - Proceedings

A2 - Petrosyan, L. A.

A2 - Zhabko, A. P.

PB - Institute of Electrical and Electronics Engineers Inc.

T2 - International Conference on "Stability and Control Processes" in Memory of V.I. Zubov, SCP 2015

Y2 - 5 October 2015 through 9 October 2015

ER -

ID: 3987245