Analysis of magnitude-color diagrams of stellar clusters.

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.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.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.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
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