ASTR 4008 / 8008 -- Star Formation

Semester 2, 2020

PDF version of this syllabus

Class meeting times

Tuesdays and Thursdays, 1 PM - 3 PM
Duffield Lecture Theater

Topics

This course covers the basics of star formation and the transition to planet formation. We begin with a survey of the physical processes that govern star-forming clouds, including magnetohydrodyanmic turbulence, gravitational instability, non-ideal MHD effects, and radiative transfer by molecules and dust grains. We then study the star formation process starting at galactic scales and working our way down, touching on topics including: star formation laws; molecular cloud formation, evolution, and disruption; collapse, fragmentation, and the origin of the initial mass function; protostellar disks and outflows; pre-main sequence stellar evolution; massive stars and feedback; and the dispersal of disks and the onset of planet formation.

Texts

Our main reference for this class will be my book Star Formation. You can get the book in several ways:

In addition to the book, we will have supplementary readings from the research literature each week. Links are below.

Assessments

This course has three forms of assessment:

  • There will be 5 problem sets, due on the dates indicated in the schedule below. These can be submitted via the course wattle page, or on paper. The problem sets together form 40% of the total assessment, and are all weighted equally. Late submissions will be accepted, at a penalty of 5% of the credit per working day, up to one week past the original due date, at which time I will distribute solution sets.
  • Each student will give one in-class presentation summarising a paper from the recent research literature, and lead a discussion of that paper. Presentations and discussions should be approximately 30 minutes each. Every student is expected to read the paper and to submit questions / comments for discussion to the student who is leading the discussion in advance. This item is 30% of the total course grade. Assessment will be based mainly on the presentation / discussion that each student leads, but the quality of participation in discussions led by other students will be considered as well.
  • There will be an oral final exam during the exam period, which will be scheduled individually. This exam will last approximately 45 minutes, and will consist of making rough estimates, order of magnitude calculations, scaling arguments, and similar quick calculations of the type that one is likely to encounter during a discussion at a scientific conference or similar venue. The exam is worth 30% of the total course grade.

Policy on collaboration

Group work is encouraged in this course. In particular, if your understanding is lacking in places, I strongly encourage you to discuss and debate with other students to reach a better understanding. However, this should not lead to a number of students producing identical assignments. In the end, you must work through, understand, and answer the assignment questions yourself, not simply reproduce verbatim other students' work. See links for further information on ANU policies on plagiarism and collusion.

Class-by-Class Topics and Reading

Date Topic Textbook chapter Reading for presentation Homework
28 July Observing the cold ISM (recording) 1
30 July Molecular line emission Appendix A
4 Aug Observing young stars (recording) 2
6 Aug Chemistry and thermodynamics (recording) 3 Glover et al., 2010, MNRAS, 404, 2 (discussion leader: Marcus)
11 Aug Gas flows and turbulence (recording) 4
13 Aug Magnetic fields (recording) 5 Planck Collaboration, 2016, A&A, 586, A138 (discussion leader: Kelly) Problem set 1 due
18 Aug Gravitational instability (recording) 6
20 Aug Feedback (recording) 7 Kim, Kim, & Ostriker, 2018, ApJ, 859, 68 (discussion leader: Alma)
25 Aug Giant molecular clouds (recording) 8
27 Aug Galaxy-scale star formation: observations (recording) 9 Sun et al., 2018, ApJ, 860, 172 (discussion leader: Aashima)
1 Sep Galaxy-scale star formation: theory (recording) 10
3 Sep Stellar clustering (recording) 11 Krumholz et al., 2018, MNRAS, 477, 2716 (discussion leader: Yuxuan) Problem set 2 due
7 - 18 Sep: semester break
22 Sep The IMF: observations (recording) 12
24 Sep The IMF: theory (recording) 13 Da Rio et al., 2012, ApJ, 748, 14 (discussion leader: Aravind)
29 Sep Discs and outflows: observation (recording) 14
1 Oct Discs and outflows: theory (recording) 15 Kratter et al., 2014, ApJ, 708, 1585 (discussion leader: Ethan) Problem set 3 due
6 Oct Protostar formation (recording) 16
8 Oct Protostellar evolution (recording) 17 Tomida et al., 2013, ApJ, 763, 6 (discussion leader: Yangyang)
13 Oct Massive star formation (recording) 18
15 Oct The first stars (recording) 19 Susa, Hasegawa, & Tominaga, 2014, ApJ, 792, 32
20 Oct Planet formation I (Mike Ireland guest lecture) (recording)
22 Oct Planet formation II (Mike Ireland guest lecture) (recording)
27 Oct Dust processes in late stage discs (recording) 20 Problem set 4 due (data file for problem 1)
29 Oct Disc dispersal (recording) 21 van der Marel et al., 2015, A&A, 579, A106
5 Nov -- Problem set 5 due
5 - 21 Nov: exam period