© 2016 SAIt.Fundamental astrophysical parameters have been derived for Be 45, Be 55, Di 07, Feib 01, Ki 02, NGC 457 and NGC 1548 open clusters (OCs) using CCD UBV(RI)C photometric data and PPMXL database. CCD UBV(RI)C photometric data observed with the 84 cm telescope at the San Pedro Martir National Astronomical Observatory (SPMO), M exico. The cluster members and field stars in the cluster regions have separated through their Proper Motion (PM) vector point diagrams. We have used JHKs photometry of 2MAS S data taken from PPMXL catalogue to have stellar Radial Density Profile (RDP) and determine limit radius of these seven clusters. Five different Color-Magnitude diagrams ane one color-color diagram have been used together with Padova isoc...
The CCD UBV(RI)(KC) photometry of the poorly studied open clusters Juchert 9 (Juc 9) and Berkeley 97...
Aims. Astrophysical parameters (age, reddening, distance, core and cluster radii) of 14 open cluster...
Aims. Astrophysical parameters (age, reddening, distance, core and cluster radii) of 14 open cluster...
Fundamental astrophysical parameters have been derived for Be 45, Be 55, Di 07, Feib 01, Ki 02, NGC ...
Fundamental astrophysical parameters have been derived for Be 45, Be 55, Di 07, Feib 01, Ki 02, NGC ...
We have selected two poor studied open clusters with the name of Berkeley97 and Dias06 which are loc...
Fundamental astrophysical parameters have been derived for 20 open clusters (OCs) using CCD UBV(RI)(...
We have selected two poor studied open clusters with the name of Berkeley97 and Dias06 which are loc...
Fundamental astrophysical parameters have been derived for 20 open clusters (OCs) using CCD UBV(RI)(...
Fundamental astrophysical parameters have been derived for 20 open clusters (OCs) using CCD UBV(RI)(...
Fundamental astrophysical parameters have been derived for 20 open clusters (OCs) using CCD UBV(RI)(...
In this study, we carried out CCD UBV photometry of eight open clusters, ASCC 115, Collinder 421, NG...
Fundamental astrophysical parameters have been derived for 20 open clus-ters (OCs) using CCD UBV(RI)...
Aims.We present results of a photometric survey whose aim was to derive structural and astrophysical...
The CCD UBV(RI)(KC) photometry of the poorly studied open clusters Juchert 9 (Juc 9) and Berkeley 97...
The CCD UBV(RI)(KC) photometry of the poorly studied open clusters Juchert 9 (Juc 9) and Berkeley 97...
Aims. Astrophysical parameters (age, reddening, distance, core and cluster radii) of 14 open cluster...
Aims. Astrophysical parameters (age, reddening, distance, core and cluster radii) of 14 open cluster...
Fundamental astrophysical parameters have been derived for Be 45, Be 55, Di 07, Feib 01, Ki 02, NGC ...
Fundamental astrophysical parameters have been derived for Be 45, Be 55, Di 07, Feib 01, Ki 02, NGC ...
We have selected two poor studied open clusters with the name of Berkeley97 and Dias06 which are loc...
Fundamental astrophysical parameters have been derived for 20 open clusters (OCs) using CCD UBV(RI)(...
We have selected two poor studied open clusters with the name of Berkeley97 and Dias06 which are loc...
Fundamental astrophysical parameters have been derived for 20 open clusters (OCs) using CCD UBV(RI)(...
Fundamental astrophysical parameters have been derived for 20 open clusters (OCs) using CCD UBV(RI)(...
Fundamental astrophysical parameters have been derived for 20 open clusters (OCs) using CCD UBV(RI)(...
In this study, we carried out CCD UBV photometry of eight open clusters, ASCC 115, Collinder 421, NG...
Fundamental astrophysical parameters have been derived for 20 open clus-ters (OCs) using CCD UBV(RI)...
Aims.We present results of a photometric survey whose aim was to derive structural and astrophysical...
The CCD UBV(RI)(KC) photometry of the poorly studied open clusters Juchert 9 (Juc 9) and Berkeley 97...
The CCD UBV(RI)(KC) photometry of the poorly studied open clusters Juchert 9 (Juc 9) and Berkeley 97...
Aims. Astrophysical parameters (age, reddening, distance, core and cluster radii) of 14 open cluster...
Aims. Astrophysical parameters (age, reddening, distance, core and cluster radii) of 14 open cluster...