Abstract
CCD BVI Johnson–Cousins photometry of the open cluster candidates Pismis 23 and BH 222 is presented. Both the analysis of the colour-magnitude diagrams and star counts performed in the regions of these two objects support their physical reality. For Pismis 23 we derive E(B−V) = 2.0 ± 0.1, E(V−I) = 2.6 ± 0.1, a distance from the Sun d= (2.6 ± 0.6) kpc and an age of (300 ± 100) Myr, while for BH 222 we obtain E(V−I) = 2. 4 ± 0.2, d= (6.0 ± 2.7) kpc and (60 ± 30) Myr. Both objects, located beyond the Sagittarius arm, are among the most reddened and distant open clusters known in the direction towards the Galactic centre.
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Clariá, J.J., Piatti, A.E. CCD BVI Photometry of the Southern Open Clusters Pismis 23 and BH 222. Astrophysics and Space Science 290, 353–362 (2004). https://doi.org/10.1023/B:ASTR.0000032534.67599.c4
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DOI: https://doi.org/10.1023/B:ASTR.0000032534.67599.c4