Module Details |
The information contained in this module specification was correct at the time of publication but may be subject to change, either during the session because of unforeseen circumstances, or following review of the module at the end of the session. Queries about the module should be directed to the member of staff with responsibility for the module. |
Title | PHYSICS OF GALAXIES | ||
Code | PHYS373 | ||
Coordinator |
Dr AF Font Physics Andreea.Font@liverpool.ac.uk |
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Year | CATS Level | Semester | CATS Value |
Session 2018-19 | Level 6 FHEQ | First Semester | 15 |
Aims |
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Learning Outcomes |
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Interpret physically the properties of normal galaxies along the Hubble sequence | |
Account for the stellar, gas, dust and dark matter content of galaxies | |
Describe the formation and evolution of galaxies in a cosmological context. |
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Analyze the structure and dynamics of galaxies and clusters of galaxies, using advanced classical mechanics and Newtonian gravity. |
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Apply fundamental physics to calculate the dynamical state of groups and clusters of galaxies, their intracluster gas, and their dark matter content. |
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Describe large-scale structure in the Universe, the nature of the first galaxies, and their implications for dark matter and cosmology. |
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Identify, summarise and present the content of research papers relevant for the field of galactic astronomy |
Syllabus |
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1 |
1 The Structure of Galaxies Size and basic structure of the Milky Way, the galactic centre. Morphological classification of galaxies. Characteristic light profiles of spirals and ellipticals. The Content of Galaxies Ages and distributions of stellar populations. Atomic gas: the 21-cm line, atomic hydrogen in the Milky Way and other galaxies, interstellar clouds, gas motions in the ISM. Ionised gas: exciting stars, Hll regions. Abundances of other elements. Interstellar dust: extinction, reddening, scattering and infrared emission. Size, shape, nature and quantity of dust. Dynamics & Stability of Galaxies Rotation o f disc galaxies. Dark matter. The Tully-Fisher relation. Spiral structure. Velocity dispersion in elliptical galaxies and bulges. Relaxation. Time scales. Overview of bsic ideas of galaxy formation. Searches for high redshift and primeval galaxies. Evolutionary Phenomena in Galaxies Stellar populations and the spectral evolution of galaxies. The origin and evolution of the chemical elements. Dynamical evolution and interactions of the ISM. Star formation. The Butcher-Oemler effect and the faint blue population at high redshift. Interactions and mergers, hot gas in galaxy clusters, fountains, bridges, starbursts and cooling flows. Morphology - density relations. Galaxy luminosity functions. Active Galaxies Quasars, nuclea r black holes, Active Galactic Nuclei, and Unified Schemes. |
Teaching and Learning Strategies |
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Lecture - Standard lectures |
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Tutorial - Standard tutorials Tutorials should takeplace in weeks 3, 5, 7, and 11 |
Teaching Schedule |
Lectures | Seminars | Tutorials | Lab Practicals | Fieldwork Placement | Other | TOTAL | |
Study Hours |
36 Standard lectures |
4 Standard tutorials |
40 | ||||
Timetable (if known) |
Tutorials should takeplace in weeks 3, 5, 7, and 11
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Private Study | 110 | ||||||
TOTAL HOURS | 150 |
Assessment |
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EXAM | Duration | Timing (Semester) |
% of final mark |
Resit/resubmission opportunity |
Penalty for late submission |
Notes |
Seen Written Exam | 3 hours | Semester 1 | 70 | Yes | Standard UoL penalty applies | Final examination Notes (applying to all assessments) - none |
CONTINUOUS | Duration | Timing (Semester) |
% of final mark |
Resit/resubmission opportunity |
Penalty for late submission |
Notes |
Coursework | 1500-2000 words | Issued in Week 1 - Deadline We | 30 | Yes | Standard UoL penalty applies | An extended research essay on a phenomenon introduced in the module |
Recommended Texts |
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Reading lists are managed at readinglists.liverpool.ac.uk. Click here to access the reading lists for this module. Explanation of Reading List: |