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Quasi-Stellar Objects (QSOs) and Schmidt s Realization
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Quasi-Stellar Objects (QSOs) and Schmidt’s Realization.

Jan 18, 2016

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Alyson Cannon
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Page 1: Quasi-Stellar Objects (QSOs) and Schmidt’s Realization.

Quasi-Stellar Objects (QSOs) and Schmidt’s

Realization

Page 2: Quasi-Stellar Objects (QSOs) and Schmidt’s Realization.

Active Galaxies

o Galaxies that have unusually bright nucleio Can have

JetsStrong variabilityStrong radio emissionBroad emission lines (like winds)

o Most are located large distance of millions and even billions LYs away

Page 3: Quasi-Stellar Objects (QSOs) and Schmidt’s Realization.

Comparison of Spectra

Page 4: Quasi-Stellar Objects (QSOs) and Schmidt’s Realization.

Enter the AGN Zoo

Seyfert Galaxies: • Bright pointlike

nuclei• In spirals• Two types –

1) Broad lines, X-rays2) Narrow lines, IR

• Lower luminosity than quasars

Radio Galaxies:• In ellipticals• Jets and large radio

emitting lobes (ala synchrotron emission)

Blazars:• Bright, extremely

variable• Little or no emission

lines• X-rays

Page 5: Quasi-Stellar Objects (QSOs) and Schmidt’s Realization.

Spectra of the Zoo Animals

Page 6: Quasi-Stellar Objects (QSOs) and Schmidt’s Realization.

Radio Galaxy Centaurus A

Page 7: Quasi-Stellar Objects (QSOs) and Schmidt’s Realization.

Sizes of AGN

Page 8: Quasi-Stellar Objects (QSOs) and Schmidt’s Realization.

Quasars

• Quasi-stellar radio sources: Radio sources that appear pointlike in visible light

• Extremely luminous at 1011 – 1015 Lo (note that LMW ~ 1011 Lo)

• Broad and narrow spectral lines• Lots of X-rays, UV, and blue light• Rapid variations indicate that source size

is compact (around a few pcs in extent)

Page 9: Quasi-Stellar Objects (QSOs) and Schmidt’s Realization.

Aside on Quasars

Quasars are waysuper bright, andso they makeexcellent probesof gas throughoutdistant space

Page 10: Quasi-Stellar Objects (QSOs) and Schmidt’s Realization.

Lyman Alpha Forest

Page 11: Quasi-Stellar Objects (QSOs) and Schmidt’s Realization.

Quasar Spectra: Emission Lines

Page 12: Quasi-Stellar Objects (QSOs) and Schmidt’s Realization.

Quasar Hosts

Page 13: Quasi-Stellar Objects (QSOs) and Schmidt’s Realization.

Supermassive Black Holes

• How to get so much energy from so little space?!

• Infall of matter onto a BH can liberate gravitational energy to be emitted as light

Page 14: Quasi-Stellar Objects (QSOs) and Schmidt’s Realization.

Ordering the Zoo

Page 15: Quasi-Stellar Objects (QSOs) and Schmidt’s Realization.

Getting the SBH Mass

• One way to estimate the BH mass is to use the Eddington limit

• AGN are incredibly luminous, but the BH mass must be large enough so that gravity results in a net infall, hence the mass must exceed

Page 16: Quasi-Stellar Objects (QSOs) and Schmidt’s Realization.

The Unified Model

Gas material is “fed” to a central SBH by an accretion disk

The disk glows to produce high luminosities

Magnetic fields channel some gas along poles to make jets

Zoo of AGN arise because of different SBH masses, feeding rates, and viewing perspectives

Page 17: Quasi-Stellar Objects (QSOs) and Schmidt’s Realization.

Illustration of AGN

Page 18: Quasi-Stellar Objects (QSOs) and Schmidt’s Realization.

Synchrotron: Magnetic Fields and

Emission

Page 19: Quasi-Stellar Objects (QSOs) and Schmidt’s Realization.

How are ancient AGN related to galaxies

today?