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ON THE POSSIBILITY OF APPLYING THE QUASI-ISOTHERMAL STACKEL'S MODEL TO OUR GALAXY. / Gromov, A. O.; Nikiforov, I. I.; Ossipkov, L. P.

в: Baltic Astronomy, Том 24, № 2, 2015.

Результаты исследований: Научные публикации в периодических изданиях › статья

Harvard

Gromov, AO, Nikiforov, II & Ossipkov, LP 2015, 'ON THE POSSIBILITY OF APPLYING THE QUASI-ISOTHERMAL STACKEL'S MODEL TO OUR GALAXY', Baltic Astronomy, Том. 24, № 2.

APA

Gromov, A. O., Nikiforov, I. I., & Ossipkov, L. P. (2015). ON THE POSSIBILITY OF APPLYING THE QUASI-ISOTHERMAL STACKEL'S MODEL TO OUR GALAXY. Baltic Astronomy, 24(2).

Vancouver

Gromov AO, Nikiforov II, Ossipkov LP. ON THE POSSIBILITY OF APPLYING THE QUASI-ISOTHERMAL STACKEL'S MODEL TO OUR GALAXY. Baltic Astronomy. 2015;24(2).

Author

Gromov, A. O. ; Nikiforov, I. I. ; Ossipkov, L. P. / ON THE POSSIBILITY OF APPLYING THE QUASI-ISOTHERMAL STACKEL'S MODEL TO OUR GALAXY. в: Baltic Astronomy. 2015 ; Том 24, № 2.

BibTeX

@article{e129fdc98a5d43ecbee7f6c021b3e123,
title = "ON THE POSSIBILITY OF APPLYING THE QUASI-ISOTHERMAL STACKEL'S MODEL TO OUR GALAXY",
abstract = "An earlier derived quasi-isothermal Stackel's model of mass distribution in stellar systems and the corresponding formula for space density are applied to our Galaxy. The model rotation curve is fitted to HI kinematical data. The structural and scale parameters of the model are estimated and the corresponding density contours for our Galaxy are presented.",
author = "Gromov, {A. O.} and Nikiforov, {I. I.} and Ossipkov, {L. P.}",
year = "2015",
language = "English",
volume = "24",
journal = "Baltic Astronomy",
issn = "1392-0049",
publisher = "Institute of Theoretical Physics and Astronomy",
number = "2",

}

RIS

TY - JOUR

T1 - ON THE POSSIBILITY OF APPLYING THE QUASI-ISOTHERMAL STACKEL'S MODEL TO OUR GALAXY

AU - Gromov, A. O.

AU - Nikiforov, I. I.

AU - Ossipkov, L. P.

PY - 2015

Y1 - 2015

N2 - An earlier derived quasi-isothermal Stackel's model of mass distribution in stellar systems and the corresponding formula for space density are applied to our Galaxy. The model rotation curve is fitted to HI kinematical data. The structural and scale parameters of the model are estimated and the corresponding density contours for our Galaxy are presented.

AB - An earlier derived quasi-isothermal Stackel's model of mass distribution in stellar systems and the corresponding formula for space density are applied to our Galaxy. The model rotation curve is fitted to HI kinematical data. The structural and scale parameters of the model are estimated and the corresponding density contours for our Galaxy are presented.

M3 - Article

VL - 24

JO - Baltic Astronomy

JF - Baltic Astronomy

SN - 1392-0049

IS - 2

ER -

ID: 4038955