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A&A 370, 931-938 (2001)
DOI: 10.1051/0004-6361:20010268
On the stellar content of the open clusters Melotte 105, Hogg 15, Pismis 21 and Ruprecht 140
A. E. Piatti and J. J. ClariáObservatorio Astronómico, Laprida 854, 5000 Córdoba, Argentina
(Received 28 November 2000 / Accepted 30 January 2001 )
Abstract
CCD observations in the B, V and I passbands have been used to generate colour-magnitude
diagrams reaching down to
mag for two slightly characterized (Melotte 105 and Hogg 15) and
two almost unstudied (Pismis 21 and Ruprecht 140) open clusters. The sample consists of about 1300 stars
observed in fields of about 4
4
. Our analysis shows that
neither Pismis 21 nor Ruprecht 140 are genuine open clusters since no clear main sequences or
other meaningful features can be seen in their colour-magnitude diagrams. Melotte 105 and Hogg 15
are open clusters affected by
and 0.95
0.05, respectively. Their distances to
the Sun have been estimated as 2.2
0.3 and 2.6
0.08 kpc, respectively, while the
corresponding ages estimated from empirical isochrones fitted to the Main Sequence cluster
members are ~350 Myr and 300 Myr, respectively. The present data are not consistent with the
membership of the WN6 star HDE 311884 to Hogg 15.
Key words: open clusters: individual: Melotte 105, Hogg 15, Pismis 21, Ruprecht 140 -- open clusters: general -- techniques: photometric
Offprint request: A. E. Piatti, andres@mail.oac.uncor.edu
SIMBAD Objects
Tables at the CDS
© ESO 2001
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