Latest Module Specifications
Current Academic Year 2025 - 2026
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Description This module focuses on the properties of high energy galactic sources, such as pulsars and X-ray binaries, and processes leading to their formation. | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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Learning Outcomes 1. 1E147F90-0A93-0001-CCF0-165414E01C45 2. Attain a good knowledge of the techniques related to the detection of X-ray and Gamma-ray photons. 4. 7,6 5. 1 6. 1E147F90-4B91-0001-F4BA-FAE019791F2A 7. Critically discuss the high-energy emission properties of X-ray binaries. 9. 7,6,8,11 10. 2 11. 1E148E85-FEA1-0001-A882-4777C77017A8 12. Understand the physical principles of mass accretion on compact objects (black holes and neutron stars) 14. 7,6,9 15. 3 16. 1E147F91-0ACD-0001-E34C-AC4611F0BB70 17. Quantitatively describe the structure and spectra of accretion disks in their basic form 19. 7,6,9 20. 4 21. 1E147F90-78A8-0001-A1D0-1DA9141C6AE0 22. Explain current high energy cosmic ray observations, and describe their features. 24. 7,11 25. 5 26. 1E37CFAD-DD1D-0001-6091-F100FEA07200 27. Summarise the strengths and weaknesses of current theories of star formation. 29. 11 30. 6 31. 1E37CFAD-B2D3-0001-E139-10201D001BB8 32. Explain the evolution of stars of a variety of masses, from their formation to their death 34. 7,6,9 35. 7 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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All module information is indicative and subject to change. For further information,students are advised to refer to the University's Marks and Standards and Programme Specific Regulations at: http://www.dcu.ie/registry/examinations/index.shtml |
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Indicative Content and Learning Activities
High energy detectors X-ray detectors, Gev detectots, TeV detectors, Cosmic Ray detectors star formation Jeans instability; Stages of gravitational contraction. X-ray binaries Low and high mass X-ray binaries; gamma-ray binaries, colliding wind binaries pulsars Various models of radio, X-ray and gamma-ray pulsars. stellar evolution difference between the evolution of low and high mass stars, degenerate gas, supernovae, compact objects | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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Indicative Reading List Books:
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Other Resources None | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||