Astronomical spectroscopy on m-type red giant stars / Mohd Hafiz bin Mohd Saadon

• Main Author: Mohd Saadon, Mohd Hafiz
• Format: Thesis
• Published: 2014
• Subjects: Q Science (General); QC Physics
• Online Access: http://studentsrepo.um.edu.my/4894/1/01._Front.pdf; http://studentsrepo.um.edu.my/4894/2/02._Declaration.pdf; http://studentsrepo.um.edu.my/4894/3/03._Abstract.pdf; http://studentsrepo.um.edu.my/4894/4/04._Contents.pdf; http://studentsrepo.um.edu.my/4894/5/05._LIST_OF_FIGURE.pdf; http://studentsrepo.um.edu.my/4894/6/06._Chapter_1.pdf; http://studentsrepo.um.edu.my/4894/7/07._Chapter_2.pdf; http://studentsrepo.um.edu.my/4894/8/08._Chapter_3.pdf; http://studentsrepo.um.edu.my/4894/9/09._Chapter_4.pdf; http://studentsrepo.um.edu.my/4894/10/10._Chapter_5.pdf; http://studentsrepo.um.edu.my/4894/11/11._Chapter_6.pdf; http://studentsrepo.um.edu.my/4894/12/12._REFERENCES.pdf; http://studentsrepo.um.edu.my/4894/13/13._APPENDICES.pdf; http://studentsrepo.um.edu.my/4894/

Red giant phase is one of the phases in stellar evolutionary tracks. The main focus of the study is to explore the late M-type red giant stars by using astronomical spectroscopy technique. Astronomical spectroscopy method is used in order to understand the chemical abundances and the pattern and cha...