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Journal of Astrophysics and Astronomy
Article . 1988 . Peer-reviewed
License: Springer TDM
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https://dx.doi.org/10.1007/bf0...
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Kinematical distances to open star clusters

descriptionPublicationkeyboard_double_arrow_right Article 01 Jun 1988 English Publisher:Springer Science and Business Media LLCJournal:Journal of Astrophysics and Astronomy, volume 9, pages 117-124 (issn: 0250-6335, eissn: 0973-7758, Copyright policy )
Authors: Ram Sagar; Harish C. Bhatt;

doi: 10.1007/bf02715688

Kinematical distances to open star clusters

Abstract

Kinematical distances are estimated for six open star clusters. They agree fairly well with the photometric distances. The kinematical distances cannot, at present, be estimated better than the photometric distances. When more accurate proper motion measurements become available the kinematical distances will improve considerably and may then be used to calibrate the cosmic distance scale.

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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).
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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.
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