Introduction to Astrophysics Lecture 17: Cosmology: the expansion of the Universe.
Announcements Pick up graded tests Homework 12 due today Pick up Homework 13 Second project is due a week from Friday If you’re following our syllabus,
15.4 Quasars and Other Active Galactic Nuclei Our Goals for Learning What are quasars? What is the power source for quasars and other active galactic nuclei?
Lecture 9: Light the Messenger Astronomy 1143 Spring 2014.
Warm Molecular Gas in Galaxies Rui-Qing Mao ( 毛瑞青 ) (Purple Mountain Observatory, Nanjing) C. Henkel (MPIfR) R. Mauersberger (IRAM) Dinh-Van-Trung (ASIAA)
Cool gas in the distant Universe Epoch of galaxy assembly (z~1 to 5) Massive galaxy formation: imaging hyper-starbursts Main sequence galaxies: gas.
Activity 1: The Sun: Source of Heat & Light Module 19: The Sun Swinburne Online Education Exploring the Solar System © Swinburne University of Technology.
Study Guide Beginning Astronomy. You must know these things: Earth's diameter is about 8000 miles Moon's distance is about 60 Earth radii (240,000 miles)
Supernova Remnants in the ChASeM33 X-ray Observations of M33 Knox Long, Bill Blair, Frank Winkler, Terry Gaetz, David Helfand, Jack Hughes, Kip Kuntz,
Massive Star Clusters in Non- Interacting Galaxies Dynamical Mass Estimates and the (I)MF Søren S. Larsen ESO / ST-ECF, Garching Tom Richtler, Concepcion.
GALEX UV Light-curves of M-Dwarf Flare Stars: “ THE FLARING UV SKY” Barry Welsh, Jonathan Wheatley & Stanley Browne (UC Berkeley) Richard Robinson (Catholic.
ELT Stellar Populations Science Near IR photometry and spectroscopy of resolved stars in nearby galaxies provides a way to extract their entire star formation.
