The compact stars - white dwarfs, neutron stars, and black holes - are the end state of stellar evolution. The conditions in and around these objects are extreme as compared to terrestrial standards, and they are responsible for some of the most powerful and dynamic phenomena in the universe. This course introduces the physics of strong gravity and dense matter required to understand compact stars and their observational manifestations.

UVa staff and guest speakers discuss current research problems.

This interdisciplinary course will introduce advanced undergraduates and graduates to molecules and their chemistry in different sources throughout the universe. Topics include gas-phase and grain-surface reactions, astronomical spectroscopy, laboratory experiments, and astrochemical modeling.Prerequisite: There are no formal prerequisites, but some knowledge of chemical kinetics, spectroscopy, and/or the interstellar medium will be helpful.

Computational methods are widely applied in all areas of astrophysical research, including data analysis, instrumentation, and theory. This course covers advanced computing skills that optimize the scientific return from using increasingly complex code bases and sophisticated code development tools. Using Python, we introduce widely applicable numerical methods while training the students in the use of commonly used code development concepts.

The course explores the formation, evolution, and properties of galaxies. Topics include: the structure of galaxies; galaxy demographics; star motions and populations; nuclear black holes; galaxy interactions; dark matter halos; the distribution of the elements; and the formation and evolution of galaxies. The course is divided equally between lecture material and project-driven worksheets.

Optional one hour laboratory for students in ASTR 3880 that provides practical experience in accessing and analyzing data related to the origin and geology of solar system planetary bodies, including the Moon, Mars, and outer planet satellites.

Primarily for astronomy/astrophysics majors. Students will be exposed to a research methods-intensive set of mini projects, with emphasis on current active areas of astrophysics research. The goal is to prepare students for research in astrophysics. Topics will include databases and database manipulation, astronomical surveys, statistics, space observatories and observation planning, intro to numerical simulations, and proposal writing.Prerequisites: ASTR 2110/2120 and PHYS 2660, or instructor permission.

The compact stars - white dwarfs, neutron stars, and black holes - are the end state of stellar evolution. The conditions in and around these objects are extreme as compared to terrestrial standards, and they are responsible for some of the most powerful and dynamic phenomena in the universe. This course introduces the physics of strong gravity and dense matter required to understand compact stars and their observational manifestations.

Computational methods are widely applied in all areas of astrophysical research, including data analysis, instrumentation, and theory. This course covers advanced computing skills that optimize the scientific return from using increasingly complex code bases and sophisticated code development tools. Using Python, we introduce widely applicable numerical methods while training the students in the use of commonly used code development concepts.

Independent study of a topic of special interest to the student under individual supervision by a faculty member. May be repeated once for credit. Prerequisite: Instructor permission.