Volume 388, Number 1, June II 2002
|Page(s)||179 - 188|
|Section||Galactic structure, stellar clusters, and populations|
|Published online||28 May 2002|
Instituto de Astronomía y Física del Espacio, CC 67, Suc. 28, 1428, Buenos Aires, Argentina
2 Observatorio Astronómico, Universidad Nacional de Córdoba, Laprida 854, 5000 Córdoba, Argentina
Corresponding author: A. E. Piatti, email@example.com
Accepted: 3 April 2002
We present the results of CCD BVI Johnson-Cousins photometry down to mag in the regions of the unstudied stellar groups Pismis 23 and BH 222, both projected close to the direction towards the Galactic centre. We measured V magnitude and and colours for a total of 928 stars in fields of about 4′ 4′. Pismis 23 is conclusively a physical system, since a clear main sequence and other meaningful features can be seen in the colour-magnitude diagrams. The reality of this cluster is also supported by star counts carried out within and outside the cluster field. For Pismis 23 we derive colour excesses and , a distance from the Sun of kpc ( pc) and an age of Myr (assuming solar metal content). BH 222 appears to be a young open cluster formed by a vertical main sequence and by a conspicuous group of luminous, typically red supergiant stars. We derived for this cluster a colour excess of , a distance from the Sun of kpc ( pc) and an age of Myr. The resulting reddening and distance estimates place these two young objects among the most reddened and distant open clusters known in the direction towards the Galactic centre. They are located beyond the Sagittarius arm, close to the direction where this arm probably bifurcates into two arms.
Key words: open clusters and associations: individual: Pismis 23, BH 222 / open clusters and associations: general / techniques: photometric
Based on observations made at the University of Toronto (David Dunlap Observatory) 24-inch telescope, Las Campanas, Chile.
© ESO, 2002
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