THE EFFECT OF THE PARAMETERS OF DUSTY SAGE GALAXY EVOLUTION MODELLING ON STELLAR MASS FUNCTION (SMF) AND DUST MASS FUNCTION (DMF)
Developing a theory of galaxy formation is one of the main focuses of astronomy today. To study galaxy formation, we need to model it through a supercomputer simulation and compare the results with observations. Current models of galaxy formation show significantly different results compared to...
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Main Author: | Hawaari Rifqi, Haru |
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Format: | Final Project |
Language: | Indonesia |
Online Access: | https://digilib.itb.ac.id/gdl/view/75044 |
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Institution: | Institut Teknologi Bandung |
Language: | Indonesia |
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