Standard

KINEMATICS DERIVED FROM NORTHERN AND SOUTHERN HEMISPHERES OF HUGE ASTROMETRIC CATALOGUES. / Vityazev, V.; Tsvetkov, A.

Proceedings of the Journees 2014 "Systemes de reference spatio-temporels". ред. / Z. Malkin; N. Capitaine. Главная (Пулковская) астрономическая обсерватория РАН, 2015. стр. 44-45.

Результаты исследований: Публикации в книгах, отчётах, сборниках, трудах конференций › статья в сборнике

Harvard

Vityazev, V & Tsvetkov, A 2015, KINEMATICS DERIVED FROM NORTHERN AND SOUTHERN HEMISPHERES OF HUGE ASTROMETRIC CATALOGUES. в Z Malkin & N Capitaine (ред.), Proceedings of the Journees 2014 "Systemes de reference spatio-temporels". Главная (Пулковская) астрономическая обсерватория РАН, стр. 44-45, Journees 2014 Systemes de Reference Spatio-temporels, Санкт-Петербург, Российская Федерация, 22/09/14.

APA

Vityazev, V., & Tsvetkov, A. (2015). KINEMATICS DERIVED FROM NORTHERN AND SOUTHERN HEMISPHERES OF HUGE ASTROMETRIC CATALOGUES. в Z. Malkin, & N. Capitaine (Ред.), Proceedings of the Journees 2014 "Systemes de reference spatio-temporels" (стр. 44-45). Главная (Пулковская) астрономическая обсерватория РАН.

Vancouver

Vityazev V, Tsvetkov A. KINEMATICS DERIVED FROM NORTHERN AND SOUTHERN HEMISPHERES OF HUGE ASTROMETRIC CATALOGUES. в Malkin Z, Capitaine N, Редакторы, Proceedings of the Journees 2014 "Systemes de reference spatio-temporels". Главная (Пулковская) астрономическая обсерватория РАН. 2015. стр. 44-45

Author

Vityazev, V. ; Tsvetkov, A. / KINEMATICS DERIVED FROM NORTHERN AND SOUTHERN HEMISPHERES OF HUGE ASTROMETRIC CATALOGUES. Proceedings of the Journees 2014 "Systemes de reference spatio-temporels". Редактор / Z. Malkin ; N. Capitaine. Главная (Пулковская) астрономическая обсерватория РАН, 2015. стр. 44-45

BibTeX

@inbook{b447086f5bc8432ebdb4c8dad02a6412,
title = "KINEMATICS DERIVED FROM NORTHERN AND SOUTHERN HEMISPHERES OF HUGE ASTROMETRIC CATALOGUES",
abstract = "It is shown that the kinematic analysis of the UCAC4, PPMXL and XPM proper motions in northern and southern Galactic hemispheres detects retardation of the Galaxy{\textquoteright}s rotational velocity and acceleration of the expansion velocity of the stellar system with increasing the distance from the principal Galactic plane. The estimates of the vertical gradient of the Galactic rotation are UCAC4: 40:1 § 0:2; PPMXL: 36:2 § 0:4; XPM: 37:7 § 0:1 km ¢ s¡1 ¢ kpc¡1, while the values of the vertical gradient of the expansion velocity turned out to be UCAC4: 11:9 § 0:2; PPMXL: 19:0 § 1:1; XPM: 10:9 § 0:3 km ¢ s¡1 ¢ kpc¡1.",
keywords = "stellar kinematics",
author = "V. Vityazev and A. Tsvetkov",
year = "2015",
language = "English",
pages = "44--45",
editor = "Malkin, { Z. } and Capitaine, {N. }",
booktitle = "Proceedings of the Journees 2014 {"}Systemes de reference spatio-temporels{"}",
publisher = "Главная (Пулковская) астрономическая обсерватория РАН",
address = "Russian Federation",
note = "Journees 2014 Systemes de Reference Spatio-temporels ; Conference date: 22-09-2014 Through 24-09-2014",
url = "http://www.gao.spb.ru/english/as/j2014/home.htm",

}

RIS

TY - CHAP

T1 - KINEMATICS DERIVED FROM NORTHERN AND SOUTHERN HEMISPHERES OF HUGE ASTROMETRIC CATALOGUES

AU - Vityazev, V.

AU - Tsvetkov, A.

PY - 2015

Y1 - 2015

N2 - It is shown that the kinematic analysis of the UCAC4, PPMXL and XPM proper motions in northern and southern Galactic hemispheres detects retardation of the Galaxy’s rotational velocity and acceleration of the expansion velocity of the stellar system with increasing the distance from the principal Galactic plane. The estimates of the vertical gradient of the Galactic rotation are UCAC4: 40:1 § 0:2; PPMXL: 36:2 § 0:4; XPM: 37:7 § 0:1 km ¢ s¡1 ¢ kpc¡1, while the values of the vertical gradient of the expansion velocity turned out to be UCAC4: 11:9 § 0:2; PPMXL: 19:0 § 1:1; XPM: 10:9 § 0:3 km ¢ s¡1 ¢ kpc¡1.

AB - It is shown that the kinematic analysis of the UCAC4, PPMXL and XPM proper motions in northern and southern Galactic hemispheres detects retardation of the Galaxy’s rotational velocity and acceleration of the expansion velocity of the stellar system with increasing the distance from the principal Galactic plane. The estimates of the vertical gradient of the Galactic rotation are UCAC4: 40:1 § 0:2; PPMXL: 36:2 § 0:4; XPM: 37:7 § 0:1 km ¢ s¡1 ¢ kpc¡1, while the values of the vertical gradient of the expansion velocity turned out to be UCAC4: 11:9 § 0:2; PPMXL: 19:0 § 1:1; XPM: 10:9 § 0:3 km ¢ s¡1 ¢ kpc¡1.

KW - stellar kinematics

UR - https://syrte.obspm.fr/jsr/journees2014/pdf/Vityazev2.pdf

UR - https://syrte.obspm.fr/jsr/journees2014/pdf/

M3 - Article in an anthology

SP - 44

EP - 45

BT - Proceedings of the Journees 2014 "Systemes de reference spatio-temporels"

A2 - Malkin, Z.

A2 - Capitaine, N.

PB - Главная (Пулковская) астрономическая обсерватория РАН

T2 - Journees 2014 Systemes de Reference Spatio-temporels

Y2 - 22 September 2014 through 24 September 2014

ER -

ID: 4736293