A new open cluster binary system in the Milky Way

Piatti A. E.; Clariá J. J.; Ahumada A. V.

Vol. 40 No. 1 (2011), Contributions

Vol. 40 No. 1 (2011)

Contributions

A new open cluster binary system in the Milky Way

Piatti A. E.⁺⁻
Clariá J. J.⁺⁻
Ahumada A. V.⁺⁻

Piatti A. E.

IAFE, CC 67, Suc. 28, CP 1428, Buenos Aires, Argentina

Clariá J. J.

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Ahumada A. V.

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Keywords

Galaxy: general
Galaxy: open clusters and associations: general
techniques: photometric

How to Cite

A new open cluster binary system in the Milky Way. (2011). Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias, 40(1), 286-286. https://astronomia.unam.mx/journals/rmxac/article/view/2011rmxac..40..286p

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Abstract

We have obtained CCD UBVI_{KC} photometry for the open clusters (OCs) Hogg 12 and NGC 3590. Based on photometric and morphological criteria, as well as on the stellar density in the region, our evidence is sufficient to consider them a new open cluster binary system candidate.

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A new open cluster binary system in the Milky Way

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