Active Galactic Nuclei Ay 16 April 8 2008

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Active Galactic Nuclei Ay 16, April 8, 2008

Active Galactic Nuclei Ay 16, April 8, 2008

AGN DEFINITION PROPERTIES GRAVITATIONAL LENSES BLACK HOLES MODELS

AGN DEFINITION PROPERTIES GRAVITATIONAL LENSES BLACK HOLES MODELS

WHAT IS AN AGN? Objects that emit significant amounts of radiation from non-thermal sources

WHAT IS AN AGN? Objects that emit significant amounts of radiation from non-thermal sources (i. e. not stars or dust or thermal gas). In order of discovery: Seyfert Galaxies Radio Galaxies Quasars BL Lac Objects LINERS (Low Ionization Emission Regions)

Early History Carl Seyfert & strange emission line galaxies (1943) Birth of Radio Astronomy

Early History Carl Seyfert & strange emission line galaxies (1943) Birth of Radio Astronomy & discovery of strong sources = radio galaxies (40 -50’s) Greenstein & Schmidt & QSO’s (1963) Surveys of Extremely Blue Objects (60 -70’s) Surveys at other Wavelengths (70’s > )

SY 1 AGN Spectra SY 2 QSO

SY 1 AGN Spectra SY 2 QSO

Mean UV QSO Spectrum

Mean UV QSO Spectrum

LBQSO Spectrum

LBQSO Spectrum

NGC 4151 Typical SY 1

NGC 4151 Typical SY 1

Seyfert 1 galaxy and quasar spectra are dominated by broad line regions, lines often

Seyfert 1 galaxy and quasar spectra are dominated by broad line regions, lines often showing doppler velocities of 0. 1 c Seyfert 2 galaxies spectra are dominated by narrower lines, ~ 1 -2000 km/s wide LINER spectra are dominated by stars plus emission lines from multiple ionization states indicative of non-thermal excitation BL Lac spectra show almost no features but strong continua

M 87 Core In X-rays

M 87 Core In X-rays

Markarian 231

Markarian 231

Markarian 421 BL Lac in an E Galaxy Te. V Source

Markarian 421 BL Lac in an E Galaxy Te. V Source

BL LAC • SED’s

BL LAC • SED’s

Radio Galaxies M 87 = Virgo A

Radio Galaxies M 87 = Virgo A

M 87 in the Radio (VLA)

M 87 in the Radio (VLA)

M 87 Central Jet

M 87 Central Jet

M 87 Jet In 3 bands

M 87 Jet In 3 bands

Centaurus A Radio on Optical Image

Centaurus A Radio on Optical Image

Cygnus A (VLA Conway & Blanco)

Cygnus A (VLA Conway & Blanco)

Synchrotron Power = related to kinetic enegy of electron = (1 - (v/c)2)-1/2 =

Synchrotron Power = related to kinetic enegy of electron = (1 - (v/c)2)-1/2 = (1 - 2)-1/2 where = v/c

Synchrotron Spectra

Synchrotron Spectra

AGN NORMAL LINERS Baldwin, Phillips & Terlevich

AGN NORMAL LINERS Baldwin, Phillips & Terlevich

Ly Alpha Forest

Ly Alpha Forest

Eddington Luminosity Largest Luminosity that can pass through a gas in hydrostatic equilibrium :

Eddington Luminosity Largest Luminosity that can pass through a gas in hydrostatic equilibrium : Outward Force of Radiation Pressure > Inward Force of Gravity d. P/dr = - g = -GM /r 2 Luminosity d. P/dr = -( T /mpc) (L/4 r 2) T = Thomson Cross section LEdd = 4 GMmpc/ T = 3. 3 x 104 L (M/M )

Gravitational Lensing Deflection of Light passing at a distance b by an object of

Gravitational Lensing Deflection of Light passing at a distance b by an object of mass M: = 4 GM/bc 2 Bending of light by the Sun: r = 6. 96 x 1010 cm M = 1. 989 x 1033 g = 8. 47 x 10 -6 radians = 1. 74”

Gravitational lensing:

Gravitational lensing:

2237+0305 = Einstein’s Cross

2237+0305 = Einstein’s Cross

Gravitational Redshift Photons lose E as the move out of a gravity well. For

Gravitational Redshift Photons lose E as the move out of a gravity well. For a photon E = hc/ , “m” = E/c 2 = h/c Gravitational Potential E = -GMm/r E = -GMh/c r / = GM/rc 2 which generally is pretty small except for NS and BH

Black Holes Curvature around a point mass has a critical radius = Schwarzchild Radius

Black Holes Curvature around a point mass has a critical radius = Schwarzchild Radius Inside this is a singularity RS = 2 GM/c 2 In units we know RS = 3. 0 km (M/M ) Gravitational redshift from RS =

NGC 4261 X-ray vs Optical

NGC 4261 X-ray vs Optical

 V = 1100 km/s

V = 1100 km/s

M 87’s central mass: Given the HST observations, what’s the enclosed mass? v =

M 87’s central mass: Given the HST observations, what’s the enclosed mass? v = 1100 km/s ~ 1” D = 16. 1 Mpc R = 0. 078 kpc (78 pc) GMm/R = 1/2 m. V 2 for circular orbits M = 0. 5 V 2 R/G G = 4. 309 x 10 -6 kpc (km/s)2 / M Mcore ~ 1010 M

Reverberation Mapping NGC 5548

Reverberation Mapping NGC 5548

Lag ~ 20 days Size ~ 20 light days ~ 0. 02 pc

Lag ~ 20 days Size ~ 20 light days ~ 0. 02 pc

Maggorian Relation (Nuker team) Almost every large galaxy has a central BH, and the

Maggorian Relation (Nuker team) Almost every large galaxy has a central BH, and the BH mass is directly correlated with the galaxy’s total bulge mass!

A Unified Model of AGN’s We have come to believe that all AGN are

A Unified Model of AGN’s We have come to believe that all AGN are essentially driven by the same phenomena --- a central black hole surrounded by an accretion disk, hot clouds of gas and dust. The disk is hot, 105 K plus. The AGN is powered by accretion onto the BH. And what you actually see is driven by the viewing angle.

Unified AGN Model BH + Disk + Torus SY 2 SY 1 BL Lac

Unified AGN Model BH + Disk + Torus SY 2 SY 1 BL Lac edge on tilted down the pipe