Astronomy 406: Fall 2020
Stellar Structure and Evolution
The goal of this course is to give students a “physical understanding” of stellar structure, star formation and evolution. We will try to explain basic concepts in simple, sometimes intuitive, physical terms. In the lectures, we will cover many topics about stars in general (not on “solar physics”), including:
- global properties (energetics and timescales)
- micro-physics (EOS, nuclear reactions, energy transport and opacity)
- equations of internal structure
- evolution as a function of stellar mass
- end states (white dwarfs, neutron stars, and black holes)
- binary interactions
This course is designed for Astronomy and Physics majors. You must have completed ASTR320 (Theoretical Astrophysics) or obtained permission from the Astronomy Department.
Schedule
Instructor: Massimo Ricotti Class: ATL 2324 Lectures: Tuesday and Thursday from 12:30pm to 13:45pm First class: Tue Sep 1 Last class: Thu Dec 10
What's New?
Sep 1: First class on zoom (check ELMS) |
Contact info and Notes
- Office: Physical Sciences Complex (PSC) 1156
- E-mail: ricotti "at" umd "dot" edu
- Phone: (301) 405 5097
- Office hours: Friday 10:00am-11:00am or by appointment
- Class web page: http://www.astro.umd.edu/~ricotti/NEWWEB/teaching/ASTR406_20.html
Course Outline
The Syllabus is available on ELMS and here PDF format.
Date | Lecture | |
---|---|---|
Basic Principles | ||
#1 | Sep 1 | Course Introduction; observations of stellar parameters, H-R diagram |
#2 | Sep 3 | Hydrostatic equilibrium and virial theorem |
#3 | Sep 8 | Gas physics: EOS |
#4 | Sep 10 | Opacities in stars |
#5 | Sep 15 | Radiative transport |
#6 | Sep 17 | Convective transport |
#7 | Sep 22 | Nuclear fusion; the s- and r-processes |
#8 | Sep 24 | Summary: stellar timescales |
#9 | Sep 29 | Equations of stellar structure, polytrophs, Lane-Emden equation |
#10 | Oct 1 | Calculating stellar evolution, the MESA code |
- | Oct 6 | MIDTERM EXAM |
Star Formation and Stellar Evolution | ||
#11 | Oct 8 | Star formation |
#12 | Oct 15 | The main sequence |
#13 | Oct 20 | Post main sequence evolution |
#14 | Oct 22 | Stellar winds mass loss |
#15 | Oct 27 | Red giant phase |
#16 | Oct 29 | Horizontal branch stars |
#17 | Nov 3 | Asymptotic giant branch stars |
Late evolution and stellar remnants | ||
#18 | Nov 5 | Post-AGB and Planetary nebulae |
#19 | Nov 10 | White dwarfs and neutron stars |
#20 | Nov 12 | Pulsating stars |
#21 | Nov 17 | Observational evidence of mass loss |
#22 | Nov 19 | Evolution of massive stars 8-25 Msun |
#23 | Nov 24 | Evolution of massive stars >25 Msun |
- | Nov 26 | THANKSGIVING (no class) |
#24 | Dec 1 | Supernovae |
#25 | Dec 3 | Close binaries and mass transfer (X-ray binaries, novae, CVs) |
#26 | Dec 8 | Chemical yields |
#27 | Dec 10 | Review session |
- | Dec 21 | FINAL EXAM (official date/time: 1:30pm-3:30pm; format and time TBD) |
Textbooks
- Required textbook:
- Understanding Stellar Evolution
by Lamers & Levesque
IOP Astronomy ebook [must log-in from UMd network to get free access] - This is a free book available in pdf, ePub and Kindle formats. Slides and exercises are also available from the same publisher. I will rely mainly on this ebook and the accompanying slides in addition to other material, mainly from Max Pettini’s lectures at IoA Cambridge (that I will make available on ELMS).
- Class participation/Quizzes 15%
- Homework 35%
- Midterm exam 25%
- Final exam 25%
- A 100% - 90%
- B 89.9% - 80%
- C 79.9% - 70%
- D 69.9% - 60%
- F below 60%
Course Grading
Homework
Homework will be assigned approximately every other week (total of 5 homework). Their due dates will be announced at the time they are assigned. On the due date the students will be expected to upload the HW on ELMS. The homework turned in will be graded and returned to the students. I will provide solutions and discuss them in class.
I will post the HOMEWORK and solutions on ELMS
Wiki pages related to class's discussions
Class #1 |