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The symposium The Inner Regions of Quasars will be held Friday, September 12th through Sunday, September 14th, 2014 on the 15th floor of Robert Lee Moore Hall (RLM) [map] on the campus of The University of Texas at Austin, to celebrate the work and career of Dr. Beverley Wills.

Broad emission lines are one of the defining criteria of all AGNs, over some 8 orders of magnitude in source luminosity. The lines orginate in the Broad Line Region (BLR) in gas that is being photoionized by the central source and moves at velocities from 1,000 to nearly 30,000 km/s. While photoionization models are quite successful in explaining much of the observed properties of AGN emission lines, major problems still remain: What is the origin of the BLR gas? What is its fate? What sets how the main gas properties, like velocity, density and location, scale with luminosity? Given the important new developments in space and ground-based spectroscopy, the time is ripe to try and answer some of these questions.

Bev Wills has been one of the pioneers in observing and interpreting the broad emission lines in all types of AGNs. Her enthusiasm and dedication inspired a generation of researchers in the field. This meeting celebrates Bev's contributions (many with Derek Wills) by presenting new results and by reviewing what has been achieved recently in this area of research.

If you have questions or information about the meeting, please direct them to the Local Organizing Committee at quasars@astro.as.utexas.edu.

Travel & Lodging

All participants are encouraged to make hotel reservations as soon as possible, as demand for lodging can be unpredictable. See Hotels for recommendations and reserved room blocks.

Registration

Please complete Registration by June 1. Registration is free. Cost of elective banquet is $45/person, payable in cash, at time of conference check-in.

Austin, Texas

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Department of Astronomy & McDonald Observatory

The Astronomy Program at The University of Texas at Austin participates in all areas of modern Astronomy, from instrumentation and device development to theoretical and computational cosmology, as well as hosting 60,000 public visitors annually at its West Texas observatory facilities.

No Registration Fee

Saturday Banquet at:

Texas Union
Eastwoods Room

UNB 2.102 (map)

SOC

Ari Laor (Chair)

Michael S. Brotherton

Hagai Netzer

Michel Breger

LOC

Michel Breger (Chair)

Joel Green

Miquela Stein

Robert Wilson

Kelly Quinney

Jim Umbarger

dr. beverley wills

Dr. Beverley Wills

Beverley J. Wills was awarded a doctoral degree in extragalactic radio astronomy from the Australian National University (Mount Stromlo Observatory and CSIRO Radiophysics), followed by a Visiting Research Scientist position in Ohio State University Electrical Engineering Department. Bev joined the Astronomy Department of the University of Texas at Austin, as a research scientist, following up, with Derek Wills, optical counterparts of sources in Jim Douglas' University of Texas Radio Astronomy Observatory's 365 MHz sky survey.

This led to several spectroscopically-related insights and investigations

  • With Hagai Netzer, the recognition of Fe II features ubiquitous in the spectra of luminous AGNs and application of Hagai's photoionization models.
  • The appearance of type I and type II AGNs spectra being the results of orientation (with others).
  • The possibility that strong scattered light could reveal buried or partially-buried AGNs, the consequent recognition of "Type II" QSOs and their contribution to the space density of AGNs. (Thanks to Michel Breger for introducing us to polarimetry.)
  • One of the largest early HST science programs to observe radio-loud quasars.
  • Investigation of the near IR spectra of QSOs led to defining the 3 micron dust-emission feature and the polarimetric separation of dust-emission, synchrotron emission in luminous radio-loud AGNs.

This journey has involved enjoyable interactions with many astronomers and astronomy students that we are partly celebrating this week.