Star clusterings in the Carina complex: UBVRI photometry of Bochum 9, 10 and 11
arXiv:astro-ph/0104195 · doi:10.1046/j.1365-8711.2001.04576.x
Abstract
We report on the first UBVRI CCD photometry of three poorly known star clusterings in the region of Eta Carinae: Bochum9, Bochum10 and Bochum11. We found that they are young, rather poor and loose open clusters. We argue that Bochum9 is probably a small and loose cluster with about 30 probable members having E(B-V)=0.63, located 4.6 kpc far from the Sun, beyond the Carina spiral arm. Similarly, Bochum10 is a sparse aggregate with 14 probable members having E(B-V)=0.47 and at a distance of 2.7 kpc from the Sun. Finally, Bochum11 is a less than 4x10^6 yrs old cluster for which we identify 24 members. It has a reddening E(B-V)=0.58, and lies between Bochum10 and 9, at 3.5 kpc from the Sun. We propose that in the field of the cluster some stars might be pre Main Sequence (MS) candidates.
12 pages, 16 figures. Accepted for publication in MNRAS
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