Standard
Kinematics of stars in old open cluster M67. /
Loktin, A. V. ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES: book. ed. / G. G. Byrd; K. V. Kholshevnikov; A. A. Myllari; I. I. Nikifirov; V. V. Orlov. Vol. 316 Astronomical Society of the Pacific, 2004. p. 163-168 (ORDER AND CHAOS IN STELLAR AND PLANETARY SYSTEMS).
Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review
Harvard
Loktin, AV 2004,
Kinematics of stars in old open cluster M67. in GG Byrd, KV Kholshevnikov, AA Myllari, II Nikifirov & VV Orlov (eds),
ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES: book. vol. 316, ORDER AND CHAOS IN STELLAR AND PLANETARY SYSTEMS, Astronomical Society of the Pacific, pp. 163-168.
APA
Loktin, A. V. (2004).
Kinematics of stars in old open cluster M67. In G. G. Byrd, K. V. Kholshevnikov, A. A. Myllari, I. I. Nikifirov, & V. V. Orlov (Eds.),
ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES: book (Vol. 316, pp. 163-168). (ORDER AND CHAOS IN STELLAR AND PLANETARY SYSTEMS). Astronomical Society of the Pacific.
Vancouver
Loktin AV.
Kinematics of stars in old open cluster M67. In Byrd GG, Kholshevnikov KV, Myllari AA, Nikifirov II, Orlov VV, editors, ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES: book. Vol. 316. Astronomical Society of the Pacific. 2004. p. 163-168. (ORDER AND CHAOS IN STELLAR AND PLANETARY SYSTEMS).
Author
Loktin, A. V. /
Kinematics of stars in old open cluster M67. ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES: book. editor / G. G. Byrd ; K. V. Kholshevnikov ; A. A. Myllari ; I. I. Nikifirov ; V. V. Orlov. Vol. 316 Astronomical Society of the Pacific, 2004. pp. 163-168 (ORDER AND CHAOS IN STELLAR AND PLANETARY SYSTEMS).
BibTeX
@inproceedings{9109f85e198c47b7b9f5547a40e26a32,
title = "Kinematics of stars in old open cluster M67",
abstract = "Preliminary results of the investigation of the kinematics of stars in open cluster M67 are discussed. This study is performed on the basis of star proper motions from a joint catalogue prepared for M67 cluster field. Cluster probable members are extracted by the use of modified Sanders method and photometric criteria. This provided us the sample of 484 probable cluster members. Radial dependence of mean radial component of stars proper motions on radius shows that most of the dependence can be attributed to the geometrical effect of convergence to radiant. Neither halo nor core of the cluster experience statistically significant expansion or contraction. Mean tangential components of proper motions reveal some hints on rotation of cluster core, but the rotation of halo is undetectable. Some properties of velocity dispersions of cluster stars are considered.",
author = "Loktin, {A. V.}",
year = "2004",
language = "English",
isbn = "1-58381-172-9",
volume = "316",
series = "ORDER AND CHAOS IN STELLAR AND PLANETARY SYSTEMS",
publisher = "Astronomical Society of the Pacific",
pages = "163--168",
editor = "Byrd, {G. G.} and Kholshevnikov, {K. V.} and Myllari, {A. A.} and Nikifirov, {I. I.} and Orlov, {V. V.}",
booktitle = "ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES",
address = "United States",
}
RIS
TY - GEN
T1 - Kinematics of stars in old open cluster M67
AU - Loktin, A. V.
PY - 2004
Y1 - 2004
N2 - Preliminary results of the investigation of the kinematics of stars in open cluster M67 are discussed. This study is performed on the basis of star proper motions from a joint catalogue prepared for M67 cluster field. Cluster probable members are extracted by the use of modified Sanders method and photometric criteria. This provided us the sample of 484 probable cluster members. Radial dependence of mean radial component of stars proper motions on radius shows that most of the dependence can be attributed to the geometrical effect of convergence to radiant. Neither halo nor core of the cluster experience statistically significant expansion or contraction. Mean tangential components of proper motions reveal some hints on rotation of cluster core, but the rotation of halo is undetectable. Some properties of velocity dispersions of cluster stars are considered.
AB - Preliminary results of the investigation of the kinematics of stars in open cluster M67 are discussed. This study is performed on the basis of star proper motions from a joint catalogue prepared for M67 cluster field. Cluster probable members are extracted by the use of modified Sanders method and photometric criteria. This provided us the sample of 484 probable cluster members. Radial dependence of mean radial component of stars proper motions on radius shows that most of the dependence can be attributed to the geometrical effect of convergence to radiant. Neither halo nor core of the cluster experience statistically significant expansion or contraction. Mean tangential components of proper motions reveal some hints on rotation of cluster core, but the rotation of halo is undetectable. Some properties of velocity dispersions of cluster stars are considered.
UR - https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=tsmetrics&SrcApp=tsm_test&DestApp=WOS_CPL&DestLinkType=FullRecord&KeyUT=000225710600029
M3 - Conference contribution
SN - 1-58381-172-9
VL - 316
T3 - ORDER AND CHAOS IN STELLAR AND PLANETARY SYSTEMS
SP - 163
EP - 168
BT - ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES
A2 - Byrd, G. G.
A2 - Kholshevnikov, K. V.
A2 - Myllari, A. A.
A2 - Nikifirov, I. I.
A2 - Orlov, V. V.
PB - Astronomical Society of the Pacific
ER -
