Active Galactic Nuclei Ay 16, April 8, 2008. AGN DEFINITION PROPERTIES GRAVITATIONAL LENSES BLACK...

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Transcript of Active Galactic Nuclei Ay 16, April 8, 2008. AGN DEFINITION PROPERTIES GRAVITATIONAL LENSES BLACK...

Active Galactic Nuclei

Ay 16, April 8, 2008

AGN

DEFINITION

PROPERTIES

GRAVITATIONAL LENSES

BLACK HOLES

MODELS

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 & 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 > )

SY1

AGN

Spectra

SY2

QSO

Mean UV QSO Spectrum

LBQSO Spectrum

NGC 4151

Typical

SY1

Seyfert 1 galaxy and quasar spectra are dominated by broad line regions, lines often showing doppler velocities of 0.1c

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

M87 Core

In

X-rays

Markarian 231

Markarian 421

BL Lac in an E Galaxy

TeV Source

BL LAC

SED’s

Radio Galaxies

M87 = Virgo A

M87 in the Radio

(VLA)

M87

Central

Jet

M87

Jet

In 3 bands

Centaurus

A

Radio on

Optical

Image

Cygnus A (VLA Conway & Blanco)

Synchrotron Power

= related to kinetic enegy of electron

= (1 - (v/c)2)-1/2 = (1 - 2)-1/2

where = v/c

Synchrotron Spectra

Baldwin, Phillips

& Terlevich

AGN

LINERS

NORMAL

Ly Alpha Forest

Eddington LuminosityLargest Luminosity that can pass through

a gas in hydrostatic equilibrium :

Outward Force of Radiation Pressure

> Inward Force of Gravity

Gravity dP/dr = -g = -GM/r2

Luminosity dP/dr = -(T/mpc) (L/4r2)

T = Thomson Cross section

LEdd = 4GMmpc/T

= 3.3 x 104 L(M/M)

Gravitational Lensing

Deflection of Light passing at a distance b by an object of mass M:

= 4GM/bc2

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:

2237+0305 = Einstein’s Cross

Gravitational Redshift

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

For a photon E = hc/, “m” = E/c2 = h/c Gravitational Potential E = -GMm/r

E = -GMh/cr

/ = GM/rc2

which generally is pretty small except for NS and BH

Black Holes

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

Inside this is a singularity

RS = 2GM/c2

In units we know

RS = 3.0 km (M/M)

Gravitational redshift from RS =

NGC 4261 X-ray vs Optical

V = 1100 km/s

M87’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 mV2 for circular orbits

M = 0.5 V2R/G

G = 4.309 x 10-6 kpc (km/s)2 / M

Mcore ~ 1010 M

Reverberation Mapping

NGC5548

Lag ~ 20 days Size ~ 20 light days ~ 0.02 pc

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 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 ModelBH + Disk + Torus

SY2 SY1 BL Lac

edge on tilted down the pipe