ANALYSIS OF THE INFLUENCE OF MASS LOSS THROUGH STELLAR WIND, ROTATION, AND OVERSHOOT ON MASSIVE STARS STRUCTURE DURING THEIR EVOLUTIONS, A REVIEW: MAIN SEQUENCE MASSIVE STARS IN SMALL MAGELLANIC CLOUDS
<p align="justify"> Massive stars have a minimum mass of 8 M? and end their lives in a supernova explosion. Scenarios from the birth to death of this star are different for each different mass ranges. In addition to mass variations, it also influenced by the evolutionary parameter...
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Main Author: | Yoshino, Hiroyuki |
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Format: | Final Project |
Language: | Indonesia |
Online Access: | https://digilib.itb.ac.id/gdl/view/75530 |
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Institution: | Institut Teknologi Bandung |
Language: | Indonesia |
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