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Strömgren-Hβ photometry of the young open cluster NGC 6913

Published online by Cambridge University Press:  31 March 2017

Nadia Kaltcheva ,
Valeri Golev ,
John Beaver ,
Steven Lund  and
Michael Briley
Nadia Kaltcheva
Affiliation:
Department of Physics and Astronomy, University of Wisconsin Oshkosh, 800 Algoma Blvd., Oshkosh, WI 54901, USA email: kaltchev@uwosh.edu
Valeri Golev
Affiliation:
Department of Astronomy, Faculty of Physics, St Kliment Ohridski University of Sofia, 5 James Bourchier Blvd., BG-1164 Sofia, Bulgaria email: valgol@phys.uni-sofia.bg
John Beaver
Affiliation:
University of Wisconsin - Fox Valley, 1874 Midway Rd, Menasha, WI, USA email: john.beaver@uwc.edu
Steven Lund
Affiliation:
Department of Physics and Astronomy, University of Wisconsin Oshkosh, 800 Algoma Blvd., Oshkosh, WI 54901, USA email: kaltchev@uwosh.edu
Michael Briley
Affiliation:
Department of Physics and Astronomy, Appalachian State University, Boone, NC 28608, USA email: brileymm@appstate.edu
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Abstract

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We present new CCD uvbyβ photometry of about 50 stars located in the central region of the open cluster NGC 6913. The individual stellar distances and color excesses of established cluster’s members are analyzed and new estimate of the cluster’s distance is provided.

Keywords

Stellar clusters and associationsuvbyβ photometryNGC 6913
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S316: Formation, evolution, and survival of massive star clusters , August 2015 , pp. 149 - 150
Copyright
Copyright © International Astronomical Union 2017 

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