We use the BCD spectrophotometric classification system to derive fundamental parameters of B stars in NGC 2439, NGC 3766 and NGC 6087. We are able to perform a complete study of each open cluster by deriving spectral classification of its members, distance modulus and age as well.Facultad de Ciencias Astronómicas y GeofísicasInstituto de Astrofísica de La Plat
Context. The knowledge of accurate values of effective temperature, surface gravity, and luminosity ...
We present CCD BVI observations obtained for stars in the fields of the unstudied or poorly studied...
The knowledge of accurate values of effective temperature, surface gravity, and luminosity of stars ...
We use the BCD spectrophotometric classification system to derive fundamental parameters of B stars ...
We use the BCD spectrophotometric classification system to derive fundamental parameters of B stars ...
Context. Spectroscopic investigations of galactic open clusters are scarce and limited to a reduced ...
Context. Spectroscopic investigations of galactic open clusters are scarce and limited to a reduced ...
International audienceContext. Stellar physical properties of star clusters are poorly known and the...
International audienceContext. Spectroscopic investigations of galactic open clusters are scarce and...
Context. Stellar physical properties of star clusters are poorly known and the cluster parameters ar...
Context. Stellar physical properties of star clusters are poorly known and the cluster parameters ar...
International audienceContext. The knowledge of accurate values of effective temperature, surface gr...
Context. Stellar physical properties of star clusters are poorly known and the cluster parameters ar...
We have obtained CCD UBVIKC photometry down to V∼ 21.0 for the open clusters Berkeley 26, Czernik 27...
Context. Stellar physical properties of star clusters are poorly known and the cluster parameters ar...
Context. The knowledge of accurate values of effective temperature, surface gravity, and luminosity ...
We present CCD BVI observations obtained for stars in the fields of the unstudied or poorly studied...
The knowledge of accurate values of effective temperature, surface gravity, and luminosity of stars ...
We use the BCD spectrophotometric classification system to derive fundamental parameters of B stars ...
We use the BCD spectrophotometric classification system to derive fundamental parameters of B stars ...
Context. Spectroscopic investigations of galactic open clusters are scarce and limited to a reduced ...
Context. Spectroscopic investigations of galactic open clusters are scarce and limited to a reduced ...
International audienceContext. Stellar physical properties of star clusters are poorly known and the...
International audienceContext. Spectroscopic investigations of galactic open clusters are scarce and...
Context. Stellar physical properties of star clusters are poorly known and the cluster parameters ar...
Context. Stellar physical properties of star clusters are poorly known and the cluster parameters ar...
International audienceContext. The knowledge of accurate values of effective temperature, surface gr...
Context. Stellar physical properties of star clusters are poorly known and the cluster parameters ar...
We have obtained CCD UBVIKC photometry down to V∼ 21.0 for the open clusters Berkeley 26, Czernik 27...
Context. Stellar physical properties of star clusters are poorly known and the cluster parameters ar...
Context. The knowledge of accurate values of effective temperature, surface gravity, and luminosity ...
We present CCD BVI observations obtained for stars in the fields of the unstudied or poorly studied...
The knowledge of accurate values of effective temperature, surface gravity, and luminosity of stars ...