<?xml version="1.0" encoding="UTF-8"?>
<course>
  <academic-career-val type="integer">1</academic-career-val>
  <assumed-knowledge-and-required-skills></assumed-knowledge-and-required-skills>
  <available-through-customised-graduate-programs type="integer" nil="true"></available-through-customised-graduate-programs>
  <co-teaching-course-id type="integer" nil="true"></co-teaching-course-id>
  <consent-description></consent-description>
  <consent-required type="boolean">false</consent-required>
  <corequisites></corequisites>
  <cost-considerations></cost-considerations>
  <course-code>ASTR3007</course-code>
  <course-description>This course will introduce star formation, structure, evolution, element production and thermonuclear reactions, and pulsating stars.&amp;nbsp; The galaxy component will cover, galaxy formation theory, classification, star formation, galaxy interactions, dark matter, black holes and large scale structure of the Universe.</course-description>
  <course-group>C</course-group>
  <eligibility></eligibility>
  <filled-flag type="integer">1</filled-flag>
  <first-year-course type="boolean">false</first-year-course>
  <id type="integer">10297</id>
  <incompatibility></incompatibility>
  <indicative-assessment>&amp;nbsp; &lt;p&gt;Stars: Three assignments, including computational problems&amp;nbsp;&amp;nbsp; 43%&lt;/p&gt;&lt;p&gt;Research essay (~1500 words + figures) and presentation to the class (~10 minutes)&amp;nbsp;&amp;nbsp;&amp;nbsp; 7%&lt;/p&gt;Galaxies: Three assignments each 15%, attendance 5%</indicative-assessment>
  <indicative-reading-list></indicative-reading-list>
  <is-active type="integer">1</is-active>
  <is-public type="integer">1</is-public>
  <learning-outcomes>For students to gain a broad scientific understanding of the following: &lt;ol&gt;&lt;li&gt;Formation, structure, evolution and pulsation of stars.&lt;/li&gt;&lt;li&gt;How are the elements produced in stars and the big bang.&lt;/li&gt;&lt;li&gt;Observational and physical properties of galaxies.&lt;/li&gt;&lt;li&gt;The structure of self-gravitating systems of many stars and gas (galaxies).&lt;/li&gt;&lt;li&gt;Dark matter, baryonic matter and galactic structure.&lt;/li&gt;&lt;li&gt;Gaining basic computer programming skills and solving problems numerically.&lt;/li&gt;&lt;/ol&gt;</learning-outcomes>
  <lock-version type="integer">6</lock-version>
  <long-title>From Stars to Galaxies</long-title>
  <max-units type="integer">6</max-units>
  <min-units type="integer">6</min-units>
  <other-information></other-information>
  <preliminary-reading></preliminary-reading>
  <prescribed-texts></prescribed-texts>
  <progress-units type="integer">6</progress-units>
  <quota></quota>
  <recommended-courses>PHYS2020, PHYS2017</recommended-courses>
  <requisite-statement>&lt;p&gt;MATH2405 or MATH2305, PHYS1201&lt;/p&gt;</requisite-statement>
  <restricted-program-entry type="integer" nil="true"></restricted-program-entry>
  <short-title>From Stars to Galaxies</short-title>
  <student-contribution-band>Band 2 NP</student-contribution-band>
  <subject>Astronomy and Astrophysics</subject>
  <technology-requirements></technology-requirements>
  <updated-by>u4046746</updated-by>
  <version type="integer">6</version>
  <workload>&lt;p&gt;Lectures and Tutorials: three lectures per week.&lt;/p&gt;</workload>
  <year type="integer">2010</year>
</course>
