| dc.contributor.author | Sserwanga, Joseph | |
| dc.date.accessioned | 2024-02-06T13:43:11Z | |
| dc.date.available | 2024-02-06T13:43:11Z | |
| dc.date.issued | 2023-08-01 | |
| dc.identifier.citation | Sserwanga, J. (2023). Analysis of Magnitude-Color Diagrams of Stellar Clusters.(Mak UD) .(Un published Undergraduate Dissertations).Makerere University ,Kampala, Uganda, Respository | en_US |
| dc.identifier.uri | http://hdl.handle.net/20.500.12281/18448 | |
| dc.description | A project report submitted to the Department of Physics in partial fulfillment of the requirements for the award of the degree of Bachelor of science with Education of Makerere University. | en_US |
| dc.description.abstract | The project aimed to estimate the ages of three stellar clusters (Melotte-72, Melotte-69, and
Berkeley-29) through analysis of their Color-Magnitude Diagrams (CMDs) using the Turn-Off
Point method with data from the Sloan Digital Sky Survey (SDSS). Age estimates were approx imately 709.2 mega years for Melotte-72 and approximately 3.18 giga years for both Melotte-69
and Berkeley-29. Since Melotte-72 is an open cluster, it’s expected to be younger than Melotte 69 and Berkeley-29 which are globular clusters. | en_US |
| dc.description.sponsorship | Uganda government | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | Makerere University | en_US |
| dc.subject | Stellar magnitudes | en_US |
| dc.subject | Color-Magnitude Diagrams (CMDs | en_US |
| dc.title | Analysis of magnitude-color diagrams of stellar clusters. | en_US |
| dc.type | Technical Report | en_US |
