This course offers an in-depth exploration of how stars form, evolve, and end their lives, integrating theoretical models with observational evidence. It begins with the physics of star formation within molecular clouds, introducing the role of gravity, turbulence, and magnetic fields in triggering stellar birth. Students will study the equations governing stellar structure, energy transport mechanisms (radiative and convective), and nuclear fusion processes powering stars at different evolutionary stages.<\/p>\n
The programme examines the Hertzsprung\u2013Russell diagram as a diagnostic tool, the classification of stellar populations, and the life cycles of stars of various masses\u2014from low-mass stars like the Sun to massive stars that end as supernovae, neutron stars, or black holes. Special attention is given to binary systems, stellar pulsations, and the interpretation of multi-wavelength and multi-messenger observations.<\/p>\n
Hands-on sessions include the analysis of real observational data, enabling students to connect theoretical predictions with actual measurements, and to familiarise themselves with the techniques used in modern astrophysics. This subject provides an essential foundation for advanced study and research in stellar astrophysics and related areas.<\/p>\n
[\/et_pb_text][et_pb_text _builder_version=”4.27.4″ _module_preset=”default” header_2_font_size=”30px” global_colors_info=”{}”]<\/p>\n
Reading List<\/h2>\n
[\/et_pb_text][et_pb_text _builder_version=”4.27.4″ _module_preset=”default” global_colors_info=”{}”]<\/p>\n
- \n
- The internal constitution of the stars.<\/em> Arthur S. Eddington. 1926. Cambridge Science Classics.<\/li>\n
- Structure and Evolution of the Stars<\/em>. M. Schwarzschild. 1958. Dover Pub. Inc., New York.<\/li>\n
- Principles of Stellar Evolution and Nucleosynthesis<\/em>. D. Clayton. 1968. McGraw Hill Inc., New York.<\/li>\n
- Stellar Structure and Evolution.<\/em> R. Kippenhahn & A. Weigert. 1990. Springer-Verlag.<\/li>\n
- The Stars<\/em>. E.L. Schatzman & F. Praderie. 1993. Springer-Verlag.<\/li>\n
- Stellar Interior<\/em>s. C.J. Hansen & S.D. Kawaler. 1994. Springer-Verlag.<\/li>\n
- Evolution of stars and stellar populations<\/em>, M. Salaris & S. Cassisi, 2005, John Wiley & Sons.<\/li>\n
- An introduction to the theory of stellar structure and evolution<\/em>, C. J. Hansen, S.D. Kawaler & V. Trimble, 2000, Cambridge University Press.<\/li>\n<\/ul>\n
[\/et_pb_text][et_pb_text _builder_version=”4.27.4″ _module_preset=”default” header_2_font_size=”30px” global_colors_info=”{}”]<\/p>\n
Teaching Plan Information<\/h2>\n
[\/et_pb_text][et_pb_image src=”https:\/\/projects.ift.uam-csic.es\/master\/wp-content\/uploads\/2025\/08\/Asignaturas-master-21-3-scaled.png” title_text=”Asignaturas m\u00e1ster (21)” url=”https:\/\/drive.google.com\/file\/d\/1v0O5JIuFaCH-y_kkwfo258wkEUxNbZ_S\/view” url_new_window=”on” _builder_version=”4.27.4″ _module_preset=”default” width=”50%” max_width=”50%” module_alignment=”center” global_colors_info=”{}”][\/et_pb_image][et_pb_text _builder_version=”4.27.4″ _module_preset=”default” header_2_font_size=”30px” custom_margin=”50px||||false|false” global_colors_info=”{}”]<\/p>\n
Course Schedule<\/h2>\n
[\/et_pb_text][et_pb_image src=”https:\/\/projects.ift.uam-csic.es\/master\/wp-content\/uploads\/2025\/08\/Asignaturas-master-20-4-scaled.png” title_text=”Asignaturas m\u00e1ster (20)” url=”https:\/\/drive.google.com\/file\/d\/1scT_JZ2cUpXDHCDLlRcfKbpO1Ru3vqMn\/view” url_new_window=”on” _builder_version=”4.27.4″ _module_preset=”default” width=”50%” max_width=”50%” module_alignment=”center” global_colors_info=”{}”][\/et_pb_image][\/et_pb_column][\/et_pb_row][\/et_pb_section]<\/p>\n","protected":false},"excerpt":{"rendered":"
Academic TeamCourse ContentType: Compulsory\u2013 AC Track \u2013 2nd Trimester This course offers an in-depth exploration of how stars form, evolve, and end their lives, integrating theoretical models with observational evidence. It begins with the physics of star formation within molecular clouds, introducing the role of gravity, turbulence, and magnetic fields in triggering stellar birth. Students […]<\/p>\n","protected":false},"author":9,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_et_pb_use_builder":"on","_et_pb_old_content":"\n
Academic Team<\/h2>\n\n\n\n
![\"\"](\"https:\/\/projects.ift.uam-csic.es\/master\/wp-content\/uploads\/2025\/08\/Asignaturas-master-14-1024x576.png\")
<\/a><\/figure>\n\n\n\n![\"\"](\"https:\/\/projects.ift.uam-csic.es\/master\/wp-content\/uploads\/2025\/08\/Asignaturas-master-27-1024x576.png\")
<\/a><\/figure>\n\n\n\nCourse Content<\/h2>\n\n\n\n
Type: Compulsory\u2013 AC Track \u2013 2nd Trimeste<\/strong>r<\/p>\n\n\n\n
This course offers an in-depth exploration of how stars form, evolve, and end their lives, integrating theoretical models with observational evidence. It begins with the physics of star formation within molecular clouds, introducing the role of gravity, turbulence, and magnetic fields in triggering stellar birth. Students will study the equations governing stellar structure, energy transport mechanisms (radiative and convective), and nuclear fusion processes powering stars at different evolutionary stages.<\/p>\n\n\n\n
The programme examines the Hertzsprung\u2013Russell diagram as a diagnostic tool, the classification of stellar populations, and the life cycles of stars of various masses\u2014from low-mass stars like the Sun to massive stars that end as supernovae, neutron stars, or black holes. Special attention is given to binary systems, stellar pulsations, and the interpretation of multi-wavelength and multi-messenger observations.<\/p>\n\n\n\n
Hands-on sessions include the analysis of real observational data, enabling students to connect theoretical predictions with actual measurements, and to familiarise themselves with the techniques used in modern astrophysics. This subject provides an essential foundation for advanced study and research in stellar astrophysics and related areas.<\/p>\n\n\n\n
Reading List<\/strong><\/h2>\n\n\n\n
- \n
- The internal constitution of the stars.<\/em> Arthur S. Eddington. 1926. Cambridge Science Classics.<\/li>\n\n\n\n
- Structure and Evolution of the Stars<\/em>. M. Schwarzschild. 1958. Dover Pub. Inc., New York.<\/li>\n\n\n\n
- Principles of Stellar Evolution and Nucleosynthesis<\/em>. D. Clayton. 1968. McGraw Hill Inc., New York.<\/li>\n\n\n\n
- Stellar Structure and Evolution.<\/em> R. Kippenhahn & A. Weigert. 1990. Springer-Verlag.<\/li>\n\n\n\n
- The Stars<\/em>. E.L. Schatzman & F. Praderie. 1993. Springer-Verlag.<\/li>\n\n\n\n
- Stellar Interior<\/em>s. C.J. Hansen & S.D. Kawaler. 1994. Springer-Verlag.<\/li>\n\n\n\n
- Evolution of stars and stellar populations<\/em>, M. Salaris & S. Cassisi, 2005, John Wiley & Sons.<\/li>\n\n\n\n
- An introduction to the theory of stellar structure and evolution<\/em>, C. J. Hansen, S.D. Kawaler & V. Trimble, 2000, Cambridge University Press.<\/li>\n<\/ul>\n\n\n\n
Teaching Plan Information<\/h2>\n\n\n\n
![\"\"](\"https:\/\/projects.ift.uam-csic.es\/master\/wp-content\/uploads\/2025\/08\/Asignaturas-master-21-1-1024x576.png\")
<\/a><\/figure>\n\n\n\nCourse Schedule<\/h2>\n\n\n\n
![\"\"](\"https:\/\/projects.ift.uam-csic.es\/master\/wp-content\/uploads\/2025\/08\/Asignaturas-master-20-1-1024x576.png\")
<\/a><\/figure>\n","_et_gb_content_width":"1080","footnotes":""},"categories":[28,30],"tags":[],"class_list":["post-1408","post","type-post","status-publish","format-standard","hentry","category-afc-track","category-compulsory-en-afc-track"],"_links":{"self":[{"href":"https:\/\/projects.ift.uam-csic.es\/master\/wp-json\/wp\/v2\/posts\/1408","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/projects.ift.uam-csic.es\/master\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/projects.ift.uam-csic.es\/master\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/projects.ift.uam-csic.es\/master\/wp-json\/wp\/v2\/users\/9"}],"replies":[{"embeddable":true,"href":"https:\/\/projects.ift.uam-csic.es\/master\/wp-json\/wp\/v2\/comments?post=1408"}],"version-history":[{"count":12,"href":"https:\/\/projects.ift.uam-csic.es\/master\/wp-json\/wp\/v2\/posts\/1408\/revisions"}],"predecessor-version":[{"id":2376,"href":"https:\/\/projects.ift.uam-csic.es\/master\/wp-json\/wp\/v2\/posts\/1408\/revisions\/2376"}],"wp:attachment":[{"href":"https:\/\/projects.ift.uam-csic.es\/master\/wp-json\/wp\/v2\/media?parent=1408"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/projects.ift.uam-csic.es\/master\/wp-json\/wp\/v2\/categories?post=1408"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/projects.ift.uam-csic.es\/master\/wp-json\/wp\/v2\/tags?post=1408"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}} - Structure and Evolution of the Stars<\/em>. M. Schwarzschild. 1958. Dover Pub. Inc., New York.<\/li>\n\n\n\n
- Structure and Evolution of the Stars<\/em>. M. Schwarzschild. 1958. Dover Pub. Inc., New York.<\/li>\n