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Stäckel-type dynamic model of the galaxy based on maser kinematic data. / Gromov, A. O.; Nikiforov, I. I.; Ossipkov, L. P.

In: Open Astronomy, Vol. 25, No. 1, 01.01.2016, p. 53-59.

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Gromov, A. O. ; Nikiforov, I. I. ; Ossipkov, L. P. / Stäckel-type dynamic model of the galaxy based on maser kinematic data. In: Open Astronomy. 2016 ; Vol. 25, No. 1. pp. 53-59.

BibTeX

@article{a6cdf631c4864177a3778c387e41314d,
title = "St{\"a}ckel-type dynamic model of the galaxy based on maser kinematic data",
abstract = "A dynamic model of the Galaxy is constructed based on kinematic data for masers with trigonometric parallaxes. Maser data is used to compute the model potential in the Galactic plane. The potential is then generalized to three dimensions assuming the existence of a third quadratic integral of motion. The resulting Galactic model potential is of St{\"a}ckel's type. The corresponding space density function is determined from Poisson's equation.",
keywords = "Galaxy: Kinematics and dynamics, Methods: Analytical",
author = "Gromov, {A. O.} and Nikiforov, {I. I.} and Ossipkov, {L. P.}",
year = "2016",
month = jan,
day = "1",
doi = "10.1515/astro-2017-0110",
language = "English",
volume = "25",
pages = "53--59",
journal = "Baltic Astronomy",
issn = "1392-0049",
publisher = "Institute of Theoretical Physics and Astronomy",
number = "1",

}

RIS

TY - JOUR

T1 - Stäckel-type dynamic model of the galaxy based on maser kinematic data

AU - Gromov, A. O.

AU - Nikiforov, I. I.

AU - Ossipkov, L. P.

PY - 2016/1/1

Y1 - 2016/1/1

N2 - A dynamic model of the Galaxy is constructed based on kinematic data for masers with trigonometric parallaxes. Maser data is used to compute the model potential in the Galactic plane. The potential is then generalized to three dimensions assuming the existence of a third quadratic integral of motion. The resulting Galactic model potential is of Stäckel's type. The corresponding space density function is determined from Poisson's equation.

AB - A dynamic model of the Galaxy is constructed based on kinematic data for masers with trigonometric parallaxes. Maser data is used to compute the model potential in the Galactic plane. The potential is then generalized to three dimensions assuming the existence of a third quadratic integral of motion. The resulting Galactic model potential is of Stäckel's type. The corresponding space density function is determined from Poisson's equation.

KW - Galaxy: Kinematics and dynamics

KW - Methods: Analytical

UR - http://www.scopus.com/inward/record.url?scp=85049259023&partnerID=8YFLogxK

U2 - 10.1515/astro-2017-0110

DO - 10.1515/astro-2017-0110

M3 - Article

AN - SCOPUS:85049259023

VL - 25

SP - 53

EP - 59

JO - Baltic Astronomy

JF - Baltic Astronomy

SN - 1392-0049

IS - 1

ER -

ID: 35488153