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DEGREE REGULATIONS & PROGRAMMES OF STUDY 2010/2011
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DRPS : Course Catalogue : School of Physics and Astronomy : Undergraduate (School of Physics and Astronomy)

Undergraduate Course: Astrophysics 3 (VS1) (PHYS10075)

Course Outline
School School of Physics and Astronomy College College of Science and Engineering
Course type Standard Availability Part-year visiting students only
Credit level (Normal year taken) SCQF Level 10 (Year 3 Undergraduate) Credits 10
Home subject area Undergraduate (School of Physics and Astronomy) Other subject area None
Course website http://www.roe.ac.uk/~pnb/teaching.html Taught in Gaelic? No
Course description Students are introduced to the physics of stars and their influence on their galactic environment. The basic observational properties of stars are reviewed including the HR diagram, followed by a discussion of the physical structure of stars on the Main Sequence to their final states as exotic objects: white dwarfs, neutron stars, and black holes. The interactions of stars with their surroundings are described - namely HII regions, stellar winds and supernova remnants.
Entry Requirements
Pre-requisites Co-requisites
Prohibited Combinations Other requirements Year 2 Physics and Mathematics
Additional Costs None
Information for Visiting Students
Pre-requisites None
Displayed in Visiting Students Prospectus? Yes
Course Delivery Information
Delivery period: 2010/11 Semester 1, Part-year visiting students only (VV1) WebCT enabled:  No Quota:  None
Location Activity Description Weeks Monday Tuesday Wednesday Thursday Friday
OtherLecture1-11 12:10 - 13:00
OtherLecture1-11 12:10 - 13:00
OtherTutorial2-11 11:10 - 13:00
First Class Week 1, Tuesday, 11:10 - 12:00, Zone: Other. ROE Lecture Theatre
Additional information Workshop/tutorial sessions, as arranged.
Exam Information
Exam Diet Paper Name Hours:Minutes Stationery Requirements Comments
Main Exam Diet S1 (December)Astrophysics 3 (VS1)2:0020 sides
Summary of Intended Learning Outcomes
Upon successful completion of this course, it is intended that the student will be able to :

1) Understand the physics behind the colour-magnitude diagram of stars.
2) Describe the physics of stellar structure, and apply hydrostatic equilibrium and radiative diffusion equations to get physical conditions and timescales.
3) Explain a star's energy production source and process, and describe how energy is transported out of a star.
4) Derive the equation of state of degenerate gas and describe the degeneracy pressure and support of white dwarfs and neutron stars.
5) Explain photoionization equilibrium, estimate the Stromgren radius and describe how the temperature and density of the intergalactic medium are measured.
6) Describe fluid dynamics equations, derive the sound speed and shock jump conditions, and explain the impact of stellar winds and supernovae on the intergalactic medium.
7) Correct for the effect on light of interstellar dust and the earth's atmosphere.
Assessment Information
Degree Examination, 100%
Special Arrangements
None
Additional Information
Academic description Not entered
Syllabus Not entered
Transferable skills Not entered
Reading list Not entered
Study Abroad Not entered
Study Pattern Not entered
Keywords As3V1
Contacts
Course organiser Dr Philip Best
Tel:
Email: pnb@roe.ac.uk
Course secretary Miss Laura Gonzalez-Rienda
Tel: (0131 6)51 7067
Email: l.gonzalez@ed.ac.uk
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copyright 2011 The University of Edinburgh - 31 January 2011 8:14 am