30 Nov 2000ASTR103, GMU, Dr. Correll1 Ch 16--Quasars and AGNs.
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Transcript of 30 Nov 2000ASTR103, GMU, Dr. Correll1 Ch 16--Quasars and AGNs.
30 Nov 2000 ASTR103, GMU, Dr. Correll 1
Ch 16--Quasars and AGNsCh 16--Quasars and AGNs
30 Nov 2000 ASTR103, GMU, Dr. Correll 2
What do you think?What do you think?
• What do quasars look like?• What powers a quasar?
30 Nov 2000 ASTR103, GMU, Dr. Correll 3
Quasars DiscoveredQuasars Discovered
• 1936--Amateur astronomer, Grote Reber, builds the first radio telescope in his backyard. He find several strong radio sources– Sagittarius A--from the galactic nucleus– Cassiopeia A--supernova remnant in our galaxy– Cygnus A--unusual
• first optical measurements were in 1951, showing a strange galaxy in the direction of the radio source
• red-shift indicated a distance of 690 million light years!
• The strong radio signal, at such a great distance, indicates a luminosity about 107 times that of a normal galaxy!
30 Nov 2000 ASTR103, GMU, Dr. Correll 4
QuasarsQuasars
optical
radio
30 Nov 2000 ASTR103, GMU, Dr. Correll 5
Quasar Red ShiftsQuasar Red Shifts
30 Nov 2000 ASTR103, GMU, Dr. Correll 6
Quasars, AGNs, etcQuasars, AGNs, etc
• Quasars--quasi stellar objects, the oldest (most distant) and most energetic galaxies
• Active Galactic Nuclei--not as far away and not as powerful as Quasars– exhibit rapid variability--indicating small energy
sources (solar system size!)– diverse spectra--some dominated by absorption, some
by emission, some featureless--classified by names such as peculiar galaxies, seyfert galaxies, BL Lac objects
– optical/xray emission near nucleus and extended radio lobes
30 Nov 2000 ASTR103, GMU, Dr. Correll 7
Seyfert Galaxy ExampleSeyfert Galaxy Example
• Ground based visible, HST visible, and x-ray reveal very localized central nucleus
30 Nov 2000 ASTR103, GMU, Dr. Correll 8
M87--Elliptical Galaxy ExampleM87--Elliptical Galaxy Example
• 50 Million light years from Earth; 3 billion solar mass nucleus (supermassive black hole?)
30 Nov 2000 ASTR103, GMU, Dr. Correll 9
Supermassive Central EnginesSupermassive Central Engines
30 Nov 2000 ASTR103, GMU, Dr. Correll 10
Radio Maps of the Milky WayRadio Maps of the Milky Way
• HST Images consistent with Supermassive black hole central engine--billion solar masses within hundreds of ly nucleus
30 Nov 2000 ASTR103, GMU, Dr. Correll 11
Gamma Ray BurstersGamma Ray Bursters
• Gamma ray detectors on satellites have discovered that many gamma ray burst sources occur.
• Recent observations confirm they are very energetic and very distant--suspected that they are energized by black hole engines, possibly capturing other black holes or neutron stars
30 Nov 2000 ASTR103, GMU, Dr. Correll 12
Gamma Ray BurstersGamma Ray Bursters
• 21-cm radiation– penetrates through the
interstellar dust to reveal spiral structure
30 Nov 2000 ASTR103, GMU, Dr. Correll 13
Quasars, AGNs, etc--SummaryQuasars, AGNs, etc--Summary
30 Nov 2000 ASTR103, GMU, Dr. Correll 14
What do you think?What do you think?
• What do quasars look like?– They look like stars, but they radiate many times more
energy than any star
• What powers a quasar?– A quasar is believed to be powered by a supermassive
black hole at the center of the galaxy