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The interstellar reddening in front of globular clusters.

descriptionPublicationkeyboard_double_arrow_right Article 01 Feb 1975 English Publisher:IOP PublishingJournal:Publications of the Astronomical Society of the Pacific, volume 87, page 65 (issn: 0004-6280, eissn: 1538-3873, Copyright policy )
Authors: D. L. Crawford; J. V. Barnes;

doi: 10.1086/129723

The interstellar reddening in front of globular clusters.

Abstract

We have observed 187 field stars in galactic fields containing globular clusters. For 15 of the 28 fields, we derive color excesses that should be essentially the same as for the globular clusters. Three additional cases deserve further work. The remaining ten fields are at low galactic latitude. To get good reddening estimates by this technique for these objects will require a selection of stars in the immediate spatial vicinity of the cluster. Key words: interstellar reddening - globular clusters

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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!
2
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