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Radial Velocity Dispersions of Star Groups in M67

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 01 Dec 2016Embargo end date: 01 Jan 2017 English Publisher:Walter de Gruyter GmbHJournal:Open Astronomy, volume 25, pages 432-438 (eissn: 2543-6376, Copyright policy )
Authors: Vereshchagin S. V.; Chupina N. V.;

doi: 10.1515/astro-2017-0263 , 10.48550/arxiv.1704.04410

arXiv: 1704.04410

Radial Velocity Dispersions of Star Groups in M67

Abstract

AbstractHigh-precision measurements of radial velocities of the M67 cluster members are used to calculate the radial-velocity dispersions in the stellar groups found earlier in the cluster’s corona. The previously detected feature in one of the groups (Group 60) consisting of stars with almost identical space velocities was confirmed. The possibility of more accurate future studies of the parameters of star groups using theGaiacatalogues is discussed.

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Keywords

open clusters and associations: individual (m 67), Astrophysics - Solar and Stellar Astrophysics, solar neighborhood, Astronomy, FOS: Physical sciences, QB1-991, Solar and Stellar Astrophysics (astro-ph.SR)

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
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