The characteristics of be star in delta scorpii system / Nazhatulshima Ahmad

• Main Author: Nazhatulshima, Ahmad
• Format: Thesis
• Published: 2013
• Subjects: Q Science (General)
• Online Access: http://studentsrepo.um.edu.my/4844/1/1_Introduction.pdf; http://studentsrepo.um.edu.my/4844/2/2_Be_stars_in_general.pdf; http://studentsrepo.um.edu.my/4844/3/3_The_program_Be_star.pdf; http://studentsrepo.um.edu.my/4844/4/4_Data_acquisition.pdf; http://studentsrepo.um.edu.my/4844/5/5_5.1Spectral_profiles_analysis_of_delta_scorpii.pdf; http://studentsrepo.um.edu.my/4844/6/6_5.3_Balmer_lines.pdf; http://studentsrepo.um.edu.my/4844/7/7_5.3.1%2DHa_var_behavior.pdf; http://studentsrepo.um.edu.my/4844/8/8%2D5.3.2.VR_variation.pdf; http://studentsrepo.um.edu.my/4844/9/9_5.3.3_Hb_and_Hg_var.pdf; http://studentsrepo.um.edu.my/4844/10/10_5.4.1_Helium_lines.pdf; http://studentsrepo.um.edu.my/4844/11/11_5.4.2Helium_lines.pdf; http://studentsrepo.um.edu.my/4844/12/12_5.5_photospheric_lines.pdf; http://studentsrepo.um.edu.my/4844/13/13_5.6_periastron_2011.pdf; http://studentsrepo.um.edu.my/4844/14/14_table5.5.pdf; http://studentsrepo.um.edu.my/4844/15/15%2D5.6_periastron_2011.pdf; http://studentsrepo.um.edu.my/4844/16/16_6.1%2DEvolutionary_study.pdf; http://studentsrepo.um.edu.my/4844/17/17_6.5_evolutionary_tracks.pdf; http://studentsrepo.um.edu.my/4844/18/18_table6.2.pdf; http://studentsrepo.um.edu.my/4844/19/19_6.5_Evolution_of_the_rotational_velocity.pdf; http://studentsrepo.um.edu.my/4844/20/20_7.Discussion.pdf; http://studentsrepo.um.edu.my/4844/21/21_Table_7.1.pdf; http://studentsrepo.um.edu.my/4844/22/22%2D7.2_Discussion2.pdf; http://studentsrepo.um.edu.my/4844/23/23%2D7.3Discussion3.pdf; http://studentsrepo.um.edu.my/4844/24/24_one%2Darm2010%2DHa.pdf; http://studentsrepo.um.edu.my/4844/25/25_one%2Darm2011%2DHa.pdf; http://studentsrepo.um.edu.my/4844/26/26_7.3Discussion4.pdf; http://studentsrepo.um.edu.my/4844/27/Abstract.pdf; http://studentsrepo.um.edu.my/4844/28/Abstrak.pdf; http://studentsrepo.um.edu.my/4844/29/acknowledgement.pdf; http://studentsrepo.um.edu.my/4844/30/appendix_B_%2Dconfig_files.pdf; http://studentsrepo.um.edu.my/4844/31/appendix_B%2Dthe_steps_EV.pdf; http://studentsrepo.um.edu.my/4844/32/appendixA%2Ddata.pdf; http://studentsrepo.um.edu.my/4844/33/Contents.pdf; http://studentsrepo.um.edu.my/4844/34/coverpage.pdf; http://studentsrepo.um.edu.my/4844/35/List_of_figures.pdf; http://studentsrepo.um.edu.my/4844/36/List_of_tables.pdf; http://studentsrepo.um.edu.my/4844/
• Institution: Universiti Malaya

Mechanisms of the disk formation in Be stars may differ from one Be star to another, which may result in the variations in the circumstellar disk’s spectral characters. The mechanism of disk formation is still under debate for the case of binary stars in which a mass transfer could not happened. -S...