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Throughout the 2021-22 academic year, we will be prioritising face to face teaching as part of a blended learning approach that builds on the lessons learned over the course of the Coronavirus pandemic. Teaching will vary between online and on-campus delivery through the year, and you should read guidance from the academic department for details of how this will work for a particular module. You can find out more about the University’s overall response to Coronavirus at: https://warwick.ac.uk/coronavirus.

PX397-7.5 Galaxies

Department
Physics
Level
Undergraduate Level 3
Module leader
Matteo Brogi
Credit value
7.5
Module duration
5 weeks
Assessment
100% exam
Study location
University of Warwick main campus, Coventry
Introductory description

A galaxy is a system of stars, dust, stellar remnants and other bodies bound by gravity. For example, the Milky Way (our galaxy) is estimated to contain around 300bn stars and at least 100bn planets. Galaxies usually form groups, also bound by their gravitational interaction, and these groups themselves tend to be part of even larger superclusters. In this module, we will see that we can put together appealing and, sometimes quite simple, explanations of what we observe in these complex systems.

Module web page

Module aims

To illustrate how important physical principles, from different areas of physics, can be developed to yield a description of complex physical systems like galaxies.

Outline syllabus

This is an indicative module outline only to give an indication of the sort of topics that may be covered. Actual sessions held may differ.

  1. Galaxy classification; the Hubble Tuning Fork; elliptical and spiral galaxies; surface
    brightness profiles.
  2. The Milky Way, its structure and properties; the role of stellar populations and the
    interstellar medium.
  3. Galaxy populations; luminosity functions, star formation vs AGN, radio galaxies and
    seyferts.
  4. Galaxy kinematics; Tully-Fisher relation; rotation curves; dark matter; virial mass
  5. The role and origin of dust and gas in galaxies; dust extinction laws; types of dusty galaxies
  6. Introduction to galaxies at large scale: the Local Group and nearby clusters
Learning outcomes

By the end of the module, students should be able to:

  • Describe the structure of our own Galaxy and how it fits into the ‘zoo’ of galaxies distributed through the Universe;
  • Explain the physical principles behind the observations used to study galaxies
  • Discuss the outstanding problems in the study of galaxies including the nature of galaxy cores and the roles of dark matter and dust
Indicative reading list

S Philipps, The Structure and Evolution of Galaxies, Wiley, 2005

View reading list on Talis Aspire

Subject specific skills

Knowledge of mathematics and physics. Skills in modelling, reasoning, thinking.

Transferable skills

Analytical, communication, problem-solving, self-study

Study time

Type Required
Lectures 15 sessions of 1 hour (20%)
Private study 60 hours (80%)
Total 75 hours
Private study description

Working through lecture notes, solving problems, wider reading, discussing with others taking the module, revising for exam, practising on past exam papers

Costs

No further costs have been identified for this module.

You must pass all assessment components to pass the module.

Assessment group B1
Weighting Study time
On-campus Examination 100%

Answer 2 questions from 3


  • Answerbook Green (8 page)
  • Students may use a calculator
Feedback on assessment

Personal tutor, group feedback

Past exam papers for PX397

Courses

This module is Option list A for:

  • Year 3 of UPXA-F304 Undergraduate Physics (BSc MPhys)
  • Year 3 of UPXA-F300 Undergraduate Physics (BSc)
  • Year 3 of UPXA-F303 Undergraduate Physics (MPhys)
  • Year 4 of UPXA-F301 Undergraduate Physics (with Intercalated Year)

This module is Option list B for:

  • UMAA-G105 Undergraduate Master of Mathematics (with Intercalated Year)
    • Year 3 of G105 Mathematics (MMath) with Intercalated Year
    • Year 5 of G105 Mathematics (MMath) with Intercalated Year
  • Year 3 of UMAA-G100 Undergraduate Mathematics (BSc)
  • UMAA-G103 Undergraduate Mathematics (MMath)
    • Year 3 of G103 Mathematics (MMath)
    • Year 4 of G103 Mathematics (MMath)
  • UMAA-G106 Undergraduate Mathematics (MMath) with Study in Europe
    • Year 3 of G106 Mathematics (MMath) with Study in Europe
    • Year 4 of G106 Mathematics (MMath) with Study in Europe
  • Year 3 of UPXA-FG33 Undergraduate Mathematics and Physics (BSc MMathPhys)
  • Year 3 of UPXA-GF13 Undergraduate Mathematics and Physics (BSc)
  • Year 3 of UPXA-FG31 Undergraduate Mathematics and Physics (MMathPhys)
  • Year 4 of UPXA-GF14 Undergraduate Mathematics and Physics (with Intercalated Year)
  • Year 4 of UMAA-G101 Undergraduate Mathematics with Intercalated Year
  • Year 3 of UPXA-F304 Undergraduate Physics (BSc MPhys)
  • Year 3 of UPXA-F303 Undergraduate Physics (MPhys)