Uvby-Beta Photometry of the Open Cluster M52

S. C. Danford; J. Thomas

Found an issue? Give us feedback

Publications of the ...arrow_drop_down

Publications of the Astronomical Society of the Pacific

Article . 1981 . Peer-reviewed

Data sources: Crossref

https://dx.doi.org/10.1086/130...

Article

Data sources: Microsoft Academic Graph

Uvby-Beta Photometry of the Open Cluster M52

descriptionPublicationkeyboard_double_arrow_right Article 01 Aug 1981 English Publisher:IOP PublishingJournal:Publications of the Astronomical Society of the Pacific, volume 93, page 447 (issn: 0004-6280, eissn: 1538-3873,

Copyright policy )

Authors: S. C. Danford; J. Thomas;

doi: 10.1086/130854

Uvby-Beta Photometry of the Open Cluster M52

- Summary
- Metrics

Abstract

Photometric uvbyβ observations of the open cluster M52 (NGC 7654) are used to determine the cluster's distance modulus (V0 - Mυ = 10.83 ± 0.24) and mean cluster reddening (E(B - V) = 0.57). The likelihood of cluster membership of the F7 Ib supergiant 60°2532 is verified on evolutionary grounds; its absolute magnitude is determined to be Mυ = -4.42 ± 0.46. The cluster M52 is shown to be similar in age to the Pleiades and the α Persei cluster.

Impact byBIP!

	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).	4
	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.	Average
	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Average
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Average