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Instructor Eric Gawiser Serin W303 Phone: 848-445-8874 Email: gawiser[at]physics.rutgers.edu Office hours: T Th 3:30-4pm
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Textbooks
There are two textbooks for this course:
Overview
Here's the official description from the course catalog:
Prerequisite: 750:507, Classical Mechanics
Properties of galaxies: photometry, structure, kinematics, gas content, chemical evolution. Structure of the Milky Way. Equilibrium, stability, and evolution of stellar systems. Dynamics and evolution of disk galaxies (spiral patterns, bars, warps) and elliptical galaxies. Examples of chaotic astrophysical systems.
I plan to broaden this list of topics to include the modern theory for how galaxies form in the context of 'hierarchical structure formation' in the Lamba Cold Dark Matter cosmological model as well as galaxies' relationships with the circumgalactic medium (CGM) and the intergalactic medium (IGM). In general, I will try to highlight subjects that are important to areas of current research in extragalactic astrophysics and cosmology (e.g., galaxy formation, the enrichment of the intergalactic medium, and the reionization of the universe).
The primary aim of this course is to establish a strong foundation of knowledge and techniques used to interpret the properties, characteristics, and dynamics of galaxies, including our own Milky Way Galaxy, galaxies in the nearby Universe, and galaxies in the distant Universe. By the end of the course students should be able to:
build a simple stellar population synthesis model for galaxies’ integrated starlight
identify different characteristics and origins of galaxies’ components and describe how they are measured
describe the evolution of gas across different temperatures, densities, and scales
diagram stellar orbits in a galaxy’s gravitational potential
concept map the theory of galaxy formation and evolution
formulate and pose fundamental questions about galaxy formation and evolution
In addition to the primary learning objectives listed above, this course’s philosophy is based on the empirically validated idea that the best learning happens through applied practice. Therefore, the primary mode of assessment in this course will not be through memorization of material, but rather through the application of knowledge and understanding to applied research problems. By the end of this course, students should be able to:
discuss the tools of an observational astronomer
solve problems computationally, and make appropriate approximations as needed
read and synthesize material from review papers with present-day literature
write a scientific proposal
share, talk, and express informed opinions about galaxies with colleagues
Both the sequence of lectures and the assignment due dates are preliminary; I will update them as needed during the course of the semester.
I will include in the schedule the dates of any local talks that are relevant to the subject matter of this course. Attendance is encouraged but not required!
| LECTURE | DATE | TOPIC | TEXT | DUE |
|---|---|---|---|---|
| 1 | Jan 20 | course overview | Ch 1,2 | |
| 2 | Jan 23 | observations: stars and stellar populations | Ch 3 | |
| 3 | Jan 27 | observations: gas and dust | ||
| 4 | Jan 29 | dwarf galaxies, satellite galaxies, and the Local Group | PS1 due Feb. 5 | |
| 5 | Feb 10 | galaxy morphologies | ||
| 6 | Feb 12 | disk galaxy kinematics: axisymmetric | Ch 4, B&T 2.6 | |
| 7 | Feb 24 | disk galaxy kinematics: bars | ||
| 8 | Feb 26 | disk galaxy kinematics: spirals | PS2 | |
| 9 | Mar 10 | galaxy centers and scaling relations | ||
| 10 | Mar 12 | elliptical galaxies: dynamics | Ch 5, B&T 2.3 | Choose proposal topic |
| 11 | Mar 17 | elliptical galaxies: stars and gas | ||
| 12 | Mar 19 | elliptical galaxies: scaling relations | PS3 | |
| 13 | Mar 24 | galaxy environments and mergers | Ch 6 | |
| 14 | Mar 26 | growth of structure in an expanding universe | Ch 7 | |
| 15 | Mar 31 | properties of dark matter halos | ||
| 16 | Apr 2 | galaxy formation | Ch 8 | Observing proposal draft |
| 17 | Apr 7 | galaxy formation: theory vs. observations | ||
| 18 | Apr 9 | active galactic nuclei (AGN) | Observing proposal peer reviews | |
| 19 | Apr 14 | the "baryon cycle": star formation and chemical evolution | Ch 9 | |
| 20 | Apr 16 | the "baryon cycle": outflows and the intergalactic medium | Ch 10 | PS4 |
| 21 | Apr 21 | high-redshift galaxies | Ch 11 | |
| 22 | Apr 23 | properties of high-redshift galaxies | Observing proposal: final version | |
| 23 | Apr 28 | galaxy dynamics oveview | B&T 1,2 | |
| 24 | Apr 30 | orbits | B&T 3 | PS5 |
| 25 | May 5 | CBE; Jeans Equation | B&T 4 | |
| 26 | May 7 | Stability considerations | B&T 5 |
Grading
Your course grade will be based on a weighted combination of four elements:
To have a given absence excused from your semester average for class participation, you must file a report at this website. To excuse a large number of absences, a note from the Dean of Students must be presented.
Homework assignments will be due in Canvas on Thursday at 11:59pm. Assignments will be of two types:
The final project will include an oral presentation (delivered in one of the last three regular class meetings) and a written paper (due at 11:59pm on May 8) on a topic relevant to extragalactic astronomy. The presentation should make use of slides and be ten minutes long. The paper should be 4-6 pages long (using a standard LaTeX template), plus figures and references in addition to the 4-6 pages of text. You may propose a topic for your final project at any time between now and March 10th, by submitting to the related Canvas Assignment your specific proposed topic and links to at least five references from the astronomical literature that you plan to use. I will approve projects on a first-come, first-serve basis; for any student who does not propose a topic of your own, I reserve the right to choose a topic for you after spring break.
Academic Integrity
Students are expected to maintain the highest level of academic integrity. You must follow the university policy on academic integrity.
Use of external sources to obtain solutions to homework assignments or exams is cheating and is a violation of the University Academic Integrity policy. Cheating in the course may result in penalties ranging from a zero on an assignment to an F for the course to expulsion from the University. Posting of homework assignments, exams, recorded lectures, or other lecture materials to external sites without the permission of the instructor is a violation of copyright and constitutes a facilitation of dishonesty, which may result in the same penalties as explicit cheating.
Not only does the use of such sites violate the University's policy on Academic Integrity, using such sites interferes with your achievement of the learning you are paying tuition for. Assignments, quizzes, and exams are given not simply to assign grades, but to promote the active learning that occurs through completing assignments on your own. Getting the right answer is much less important than learning how to get the right answer. This learning is critical to your success in subsequent courses and your careers.
Almost all original work is the intellectual property of its authors. These works include syllabi, lecture slides, recorded lectures, homework problems, exams, and other materials, in either printed or electronic form. The authors hold copyrights in these works, which are protected by U.S. statutes. Copying this work or posting it online without the permission of the author violates the author's rights. More importantly, these works are the product of the author's efforts; respect for these efforts and for the author's intellectual property rights is an important value that members of the university community take seriously.
Artificial IntelligenceAll use of Generative A/I in this course must be disclosed. You are encouraged to use spellcheckers and/or grammar checkers (e.g., Grammarly) on the Writing Assignments and Term Project papers, but you cannot use any software or websites (e.g., ChatGPT) that writes text for you. It is ok to use Generative AI to polish text that you have already written, but this must be disclosed as part of the paper or problem set where you used it.
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