Interstellar Medium 2012 Q4

Lecturer: Floris van der Tak

Assistant: Yunhee Choi

Motivation

The interstellar medium (ISM) is the place where material from old stars gets recycled into new generations of stars. The ISM thus plays a central role in the evolution of galaxies and of matter in the Universe. This course teaches the concepts necessary to understand the ISM: the physics of rarefied gases under various conditions. These concepts have applications in all branches of astrophysics.

Goals

After following the course, the student will be able to:

  1. describe the diagnostics of rarefied gases: explain what types of gas emit radiation at which wavelengths, and how the spectral lines of atoms and molecules may be used to determine the conditions of a gas;

  2. describe the heating and cooling of rarefied gases: tell the main mechanisms which influence the gas temperature and explain when which mechanisms play a role;

  3. describe the dynamics of interstellar gases: explain which processes cause motions in the gas, and when which process plays a role;

  4. describe the conditions for star formation: explain which conditions in the interstellar medium are necessary and sufficient for the formation of new stars.

These goals will be achieved at two levels: a theoretical level where the student can express insight, and a practical level where this insight is applied in calculations.

Book (required)

Physics of the Interstellar and Intergalactic Medium, Bruce T. Draine, Princeton Series in Astrophysics, ISBN 9780691122137 (hardcover) or 9780691122144 (paperback).

Prerequisites

Astrophysics B / Radiative Processes in Astrophysics: the book by Rybicki & Lightman.

Students must register for the course at least two weeks before the first lecture, i.e., by week 15. The book by Draine may take a week or more to be delivered, so it also should be ordered by week 15. Registration should be done by e-mailing Floris van der Tak, with a cc to Gineke Alberts; see below for contact info. The homework for the first lecture is to read the first chapter from Draine's book.

Format

The course consists of 2x2 hours of lectures and 1x2 hours of practical work per week, over a period of 8 weeks. Before each lecture, the students read the relevant chapter of the book. In the lectures, the course material is introduced and illustrated with examples. At the end of each lecture, the homework assignments for the following practical work session are handed out. The students prepare answers to each question in the form of a short (~1 page per subquestion) digital slide show (using PowerPoint, Keynote, OpenOffice, or a similar program) and send a PDF version by e-mail to the assistant by Thursday 12:00 noon. In the practical sessions, a randomly selected student presents his/her solution to the question, and the group discusses this solution. The quality of these presentations and participation in these discussions together form 1/4 of the grade for the course.

Exam

After the last week of lectures, there is a written exam in two parts. The first part consists of questions into knowledge and insight of the course material, which must be answered without the book. The second part consists of application-type questions which may be answered using the book. The final grade for the course is a weighted average of the grades for the exam (75%) and for the homework assignments (25%).

Schedule

The basic schedule is given on the Ocasys page but see the table below for exceptions. The chapters in column 3 are the homework for that lecture. You can skip the sections marked by (*) in the book.



Date

Topic

Book chapter

24-04-2012

I. Overview of the ISM

1, 12, 40


Part 1: Regions of ionized gas


26-04-2012

II. Pure hydrogen nebulae

3, 4, 10, 11

27-04-2012

Problem Set 1


03-05-2012

III. Nebulae with heavier elements

6, 14 (incl. 14.3), 15 (incl. 15.8)

04-05-2012

IV. Heating & cooling of H+ regions

2, 27

08-05-2012

V. Diagnostics of H+ regions

17, 18, 28

10-05-2012

VI. Non-stellar H+ regions

13, 16, 20 (incl. 20.2 & 20.3)

11-05-2012

Problem Set 2



Part 2: Regions of neutral gas


15-05-2012

VII. Observational probes of neutral gas

8, 9, 29

16-05-2012

Problem Set 3

11:00-13:00, room 257

21-05-2012

Problem Set 4

11:00-13:00, room 257

22-05-2012

VIII. Thermal balance of neutral gas

30

24-05-2012

IX. Interstellar shock waves

35, 36 (incl. 36.6)

25-05-2012

Problem Set 5


29-05-2012

X. The multi-phase ISM

34, 39


Part 3: Regions of molecular gas


31-05-2012

XI. Molecular spectra

5, 7, 19, 31

01-06-2012

Problem Set 6


05-06-2012

XII. Interstellar dust

21, 22, 23, 24, 25

06-06-2012 (257)

XIII. Diffuse molecular clouds & PDRs

32, 33

11-06-2012

Problem Set 7


12-06-2012

XIV. Dense molecular clouds & star formation

41, 42

14-06-2012

XV. The extragalactic ISM


19-06-2012

Problem Set 8


28-06-2012

Exam = deadline assignments

09:30-12:00; room 161

Contact

Floris van der Tak:

telephone (050) 363 8753

e-mail f.f.s.van.der.tak AT rug.nl

office: 5419.0294 (Kapteynborg, second floor)



Yunhee Choi:

telephone (050) 363 4276

e-mail y.choi AT astro.rug.nl

office 5419.0254 (Kapteynborg, second floor)



Gineke Alberts (Education Secretary):

telephone (050) 363 4073

e-mail m.g.alberts AT astro.rug.nl

office 5419.0178 (Kapteynborg, first floor)