Absolute uvbybeta photoelectric photometry of the brightest stars in the direction of the Open Cluster NGC 6823 has been secured and is presented. From the data analysis, reddening, distance, temperature and gravity are determined for the B, A, F stars and, from these, reddening and a mean distance modulus (12.475 +/- 0.414 mag) to the cluster are determined. Also, their membership in the cluster has been established and a numerical value of the age is determined through direct comparison with theoretical models. A brief analysis of the short period variable stars in the direction of NGC 6823 is made. We have concluded that they might not be pre-MS delta Scuti stars
Abstract. Magnitudes and colors in the UBV photometric system have been determined for 575 stars in ...
Abstract. Magnitudes and colors in the UBV photometric system have been determined for 575 stars in ...
Abstract. Magnitudes and colors in the UBV photometric system have been determined for 575 stars in ...
Photoelectric UBV magnitudes have been determined for 41 stars in NGC 6823. The reddening across the...
UBV photoelectric photometry for 175 stars in the field of the southern open cluster NGC 2323, suppl...
We present the results of CCD UBV observations of the open cluster NGC 6819. We calculated the stell...
We present CCD UBVRI photometry of the field of the open cluster NGC 6866. Structural parameters of ...
We present CCD UBVRI photometry of the field of the open cluster NGC 6866. Structural parameters of ...
Photoelectric UBV magnitudes and colours have been determined for 103 stars in the field of NGC 6913...
The thesis examines the characteristics of the clusters and their distribution in our Galaxy, the pr...
Abstract. Magnitudes and colors in the UBV photometric system have been determined for 575 stars in ...
Abstract. Magnitudes and colors in the UBV photometric system have been determined for 575 stars in ...
Abstract. Magnitudes and colors in the UBV photometric system have been determined for 575 stars in ...
We present the results of CCD UBVRI observations of the open cluster NGC 6811 obtained on 18th July ...
Abstract. Magnitudes and colors in the UBV photometric system have been determined for 575 stars in ...
Abstract. Magnitudes and colors in the UBV photometric system have been determined for 575 stars in ...
Abstract. Magnitudes and colors in the UBV photometric system have been determined for 575 stars in ...
Abstract. Magnitudes and colors in the UBV photometric system have been determined for 575 stars in ...
Photoelectric UBV magnitudes have been determined for 41 stars in NGC 6823. The reddening across the...
UBV photoelectric photometry for 175 stars in the field of the southern open cluster NGC 2323, suppl...
We present the results of CCD UBV observations of the open cluster NGC 6819. We calculated the stell...
We present CCD UBVRI photometry of the field of the open cluster NGC 6866. Structural parameters of ...
We present CCD UBVRI photometry of the field of the open cluster NGC 6866. Structural parameters of ...
Photoelectric UBV magnitudes and colours have been determined for 103 stars in the field of NGC 6913...
The thesis examines the characteristics of the clusters and their distribution in our Galaxy, the pr...
Abstract. Magnitudes and colors in the UBV photometric system have been determined for 575 stars in ...
Abstract. Magnitudes and colors in the UBV photometric system have been determined for 575 stars in ...
Abstract. Magnitudes and colors in the UBV photometric system have been determined for 575 stars in ...
We present the results of CCD UBVRI observations of the open cluster NGC 6811 obtained on 18th July ...
Abstract. Magnitudes and colors in the UBV photometric system have been determined for 575 stars in ...
Abstract. Magnitudes and colors in the UBV photometric system have been determined for 575 stars in ...
Abstract. Magnitudes and colors in the UBV photometric system have been determined for 575 stars in ...
Abstract. Magnitudes and colors in the UBV photometric system have been determined for 575 stars in ...