ASTR 5460, Fri. May 2,
2003
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Evaluations (official and unofficial) |
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Reminders/Assignments |
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Finish Quasars and Active Galactic
Nuclei |
Reminders/Assignments
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Research Homework Update |
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Dan finished phase 1, conducting phase
2 |
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Chris, Sey, and Cassandra primary now |
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Jon and Sabrina should see me soon |
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Presentation topics |
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Galex launched! |
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http://www.galex.caltech.edu/ |
Presentation Topics
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Plan for 20 minutes, plus questions. |
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Other astronomy faculty are invited. |
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Topics: |
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Gunn-Peterson Test and Reionization |
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Supernovae and the Accelerating
Universe |
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Weighing Supermassive Black Holes |
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The Hubble Deep Fields |
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Sub-millimeter (SCUBA) Galaxies |
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X-ray Background |
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Quasars and Active
Galactic Nuclei (AGNs)
The AGN “Zoo”
Orientation and Unified
Models
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“Unified Models” explain some of the
different classes of AGN, particularly type 1 and type 2 Seyferts, via
orientation. |
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For specifics, see the Annual Reviews
article by Antonucci, 1993, a “bishop” in the “Church of Unification.” |
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Another nice website:
http://www.mssl.ucl.ac.uk/www_astro/agn/agn_unified.html |
Quasar Spectral Energy
Distributions (SEDs)
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Very nice and relatively brief review
article from “Quasars and Cosmology” conference by Belinda Wilkes (CfA), a
world expert on the subject: |
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http://nedwww.ipac.caltech.edu/level5/Sept01/Wilkes/Wilkes_contents.html |
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Must account for physical processes
producing prodigious luminosity from radio wavelengths through the X-ray and
even gamma ray regimes. |
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Particular features of interest
include radio-jets and the radio-quiet vs. radio-loud dichotomy, the “big
blue bump” that produces the optical/UV energy peak and is thought to arise
from an accretion disk, and the far infrared that represents re-radiation by
hot dust. |
Quasar Spectral Energy
Distributions (SEDs)
Surveys/Catalogs
AGN Accretion
AGN Accretion Disks
AGN Emission Lines
Quasar Host Galaxies
Quasar Images II
Quasar Images III:
“Starburst-Quasar”
Ties to Host Galaxy
Evolution
Ties to Host Galaxy
Evolution
Ties to Host Galaxy
Evolution
Next Time