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The author describes how scientists can observe and draw conclusions about black holes. Scenarios of both "top down" and "bottom up" galaxy formation are discussed, together with the relationship between red and blue galaxies and dwarf, elliptical, and spheroidal galaxies. The problem of dark matter is then addressed, including its relationship to visible matter and to the structure of the universe on the grand scale, focusing on the success of the Cold Dark Matter model.

The author concludes by reviewing problems that remain to be solved and the techniques that might begin to be used to solve these. Mysteries of Galaxy Formation. He uses analytic computations, numerical simulations, and observations to discover and characterize these objects.

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With collaborators, he was the first to propose that radio observations could be used to image the shadow of the event horizon of a black hole and the first to create an infrared longitudinal map of an extrasolar planet. Along with affiliated students and postdocs, Anderson makes use of data from a variety of ground- e. Anderson teaches courses related to high energy astrophysics and radiative processes.

Galaxy Formation in a Magnetic Universe

The processes that form and shape PNe remain amount the least understood facets of stellar evolution. I use images and spectroscopy to understand an interpret their shapes and internal motions. This includes the Sun.


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Much as a butterfly emerges when its chrysalis is ejected, planetary nebulae are formed when a red giant star ejectes its outer layers as clouds of luminescent gas, revealing the dense, hot, and tiny white…. Rory Barnes is a theorist in the Virtual Planetary Laboratory primarily interested in the formation and evolution of habitable planets. He has also worked extensively on the orbital evolution of giant exoplanets, demonstrating that most multiple planets systems appear packed, meaning no more can exist between those that are known.

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My primary research interest is using the resulting massive optical variability datasets to identify rare compact binaries and to classify other sources of high energy radiation. I use the ARC 3. My work focuses on using large surveys to study cosmology and the evolution of galaxies. This ranges from studying the clustering of galaxies and their evolution with redshift, weak gravitational lensing of galaxies, and estimating the properties of galaxies based on their colors aka photometric redshifts. The common theme to this work is addressing the need for massive data sets and how to work with them.

Beyond cosmology, I am also interested in how to make the technologies that companies use to search the internet useful in research and education. Julianne Dalcanton works on galaxy formation and evolution, focusing primarily on what can be learned in the nearby universe.

Her group is currently working on several large projects studying the resolved stellar populations of nearby galaxies using HST, their neutral gas distribution with the VLA, and their stellar mass, dust, and star formation properties with Spitzer. She also works closely with the N-body shop on the interface between observation and numerical theory.

Joined UW in: grad student , lecturer.

Suzanne Hawley works in stellar astrophysics, particularly in the areas of magnetic activity, low mass stars, brown dwarfs and variable stars. In addition, she studies star clusters, the stellar content of dwarf galaxies, and galactic structure. Suzanne also serves as the Director of the ARC 3.

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My research interests include Local Group galaxies, modes of star formation, star clusters and their formation, HII regions in galaxies, meteorite craters. He obtained Ph. Studied at: University of Zagreb , University of Kentucky Major astronomical surveys of today are routinely collecting hundreds of terabytes of images, creating databases with billions of objects and several billion measurements.

Large surveys astronomers are becoming part data scientists. My current focus is using survey data to understand the structure and evolution of the Milky Way. My interests lie in teaching multi-level astronomy courses incorporating active student participation in lectures, labs, and on-line exercises, and curriculum development for these courses, including a published lecture activity book: Learning Astronomy by Doing Astronomy — Collaborative Lecture Activities. Members of the League of Astronomers and I are involved in a long-term project doing photometry of little-studied open clusters to determine stellar metallicities based on Stromgren observations at the Dominion Astrophysical Observatory in Victoria, BC.

I am involved in the outreach program here, primarily with the Jacobsen Observatory, and in teaching students how to give great scientific public talks. My primary interest is working with students — both in and out of the Astronomy major — to get all they can from their time here at the University. I dedicate most of my working hours to developing the courses I teach, and to mentoring those students who wish to extend the reach of their education beyond the classroom.

Her current research program includes panchromatic observations and models of star-forming galaxies and their young stellar populations; host galaxy and progenitor studies of massive star transients such as LBVs, supernovae, and long-duration gamma-ray bursts; surveys of evolved massive stars in and beyond the Local Group; and the properties of Thorne-Zytkow objects. Professor Lutz is interested in understanding the physical characteristics of planetary nebulae and their central stars and how these objects fit into the patterns of stellar evolution.

She also analyzes the spectra of symbiotic stars binaries containing an evolved hot star and a cool star to determine their chemical compositions, velocities and variability. She has broad interests in astronomy education, including working with K educators, museums, science centers and after-school program.

Matt is a theoretical astrophysicist and cosmologist.


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Victoria Meadows is an astrobiologist and planetary astronomer whose research interests focus on acquisition and analysis of remote-sensing observations of planetary atmospheres and surfaces. In addition to studying planets within our own Solar System, she is interested in exoplanets, planetary habitability and biosignatures.

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Her NAI team uses models of planets, including planet-star interactions, to generate plausible planetary environments and spectra for extrasolar terrestrial planets and the early Earth. This research is being used to help define signs of habitability and life for future extrasolar terrestrial planet detection and characterization missions.

Tom leads the N-body shop, where he works on running and analyzing N-body simulations of structure formation in the Universe and planet formation. His other research interests include Galactic and Solar System dynamics. He is a member of the UW Astrobiology program. Studied at: Florida Institute of Technology My primary research and teaching interests are focused on the processes that shape the surfaces of the worlds of our solar system.

In particular, my research has focused on investigating and sampling terrestrial meteorite craters to study the physical process that create and distribute meteoritic material around them. My primary teaching interests are the geological processes and history of the solar system and the history of the Apollo Lunar missions.

Recent SETI activity has included a collaboration with the Serendip group, using the Arecibo foot dish for an all-sky search for a wide variety of signal modulation at 21 cm seti home project. History of astronomy research has been on the twentieth century, in particular the development of early radio astronomy Cosmic Noise: A History of Early Radio Astronomy, and ideas about extraterrestrial life, as well as a long-term project designed to produce a biography of William Herschel.