We report on BVI CCD photometry to V = 22.0 for three fields centred on the region of the Galactic Star clusters Ruprecht 4, Ruprecht 7 and Pismis 15 and on three displaced control fields. Ruprecht 4 and Pismis 15 have never been studied before, and we provide, for the first time, estimates of their fundamental parameters, namely, radial extent, age, distance and reddening. Ruprecht 7 (Berkeley 33), however, was studied by Mazur, Kaluzny & Krzeminski. We find that the three clusters are all of intermediate age (0.8-1. 3 Gyr), and with a metallicity close to or lower than solar.Facultad de Ciencias Astronómicas y GeofísicasInstituto de Astrofísica de La Plat
Ruprecht 147 is a hitherto unappreciated open cluster that holds great promise as a standard in fund...
We present CCD observations in the B,V and I passbands obtained for stars in the fields of the open ...
Multicolour photometry of the stellar populations in five fields in the third Galactic quadrant cent...
We report on BVI CCD photometry to V = 22.0 for three fields centred on the region of the Galactic S...
We report on BVI CCD photometry to V = 22.0 for three fields centred on the region of the Galactic S...
We present the first BVI CCD photometry to V = 22.0 of four fields centred on the region of the sout...
We present the first BVI CCD photometry to V = 22.0 of four fields centred on the region of the sout...
We present the first BVI CCD photometry to V = 22.0 of four fields centred on the region of the sout...
We present CCD observations in the Washington system C and T1 passbands down to T1 ∼ 18.5 in the fie...
We derive fundamental, structural and photometric parameters of 15 overlooked Ruprecht (hereafter Ru...
We derive fundamental, structural and photometric parameters of 15 overlooked Ruprecht (hereafter Ru...
We derive fundamental, structural and photometric parameters of 15 overlooked Ruprecht (hereafter Ru...
We present CCD BVI observations obtained for stars in the fields of the unstudied or poorly studied...
CCD observations in the B, V and I passbands have been used to generate colour-magnitude diagrams re...
Ruprecht 147 is a hitherto unappreciated open cluster that holds great promise as a standard in fund...
Ruprecht 147 is a hitherto unappreciated open cluster that holds great promise as a standard in fund...
We present CCD observations in the B,V and I passbands obtained for stars in the fields of the open ...
Multicolour photometry of the stellar populations in five fields in the third Galactic quadrant cent...
We report on BVI CCD photometry to V = 22.0 for three fields centred on the region of the Galactic S...
We report on BVI CCD photometry to V = 22.0 for three fields centred on the region of the Galactic S...
We present the first BVI CCD photometry to V = 22.0 of four fields centred on the region of the sout...
We present the first BVI CCD photometry to V = 22.0 of four fields centred on the region of the sout...
We present the first BVI CCD photometry to V = 22.0 of four fields centred on the region of the sout...
We present CCD observations in the Washington system C and T1 passbands down to T1 ∼ 18.5 in the fie...
We derive fundamental, structural and photometric parameters of 15 overlooked Ruprecht (hereafter Ru...
We derive fundamental, structural and photometric parameters of 15 overlooked Ruprecht (hereafter Ru...
We derive fundamental, structural and photometric parameters of 15 overlooked Ruprecht (hereafter Ru...
We present CCD BVI observations obtained for stars in the fields of the unstudied or poorly studied...
CCD observations in the B, V and I passbands have been used to generate colour-magnitude diagrams re...
Ruprecht 147 is a hitherto unappreciated open cluster that holds great promise as a standard in fund...
Ruprecht 147 is a hitherto unappreciated open cluster that holds great promise as a standard in fund...
We present CCD observations in the B,V and I passbands obtained for stars in the fields of the open ...
Multicolour photometry of the stellar populations in five fields in the third Galactic quadrant cent...