Peculiarity of stellar kinematics in the solar vicinity

Please use this identifier to cite or link to this item: http://elar.urfu.ru/handle/10995/27318

Title:	Peculiarity of stellar kinematics in the solar vicinity
Authors:	Popova, M. E.
Issue Date:	2013
Publisher:	Astronomische Nachrichten
Citation:	Popova M. E. Peculiarity of stellar kinematics in the solar vicinity / M. E. Popova // Astronomische Nachrichten. — 2013. — Vol. 334. — № 8. — P. 756-759.
Abstract:	The peculiar velocities of nearby stars are studied. We determine the solar velocity components from the radial velocities and proper motions of stars and open clusters. We show that nearby stars are not very suitable for the determination of the solar motion components because of peculiarities in their velocity distribution. © 2013 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.
Keywords:	OPEN CLUSTERS AND ASSOCIATIONS: GENERAL SOLAR NEIGHBORHOOD STARS: KINEMATICS AND DYNAMICS
URI:	http://elar.urfu.ru/handle/10995/27318
SCOPUS ID:	84885135122
WOS ID:	000327899600004
PURE ID:	861260
ISSN:	0004-6337
DOI:	10.1002/asna.201311916
Appears in Collections:	Научные публикации ученых УрФУ, проиндексированные в SCOPUS и WoS CC

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