Peculiar colliding Galaxies and Active Galaxies Colliding galaxies

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Peculiar (colliding) Galaxies and Active Galaxies Colliding galaxies tidal distortions, star formation, evolution (role

Peculiar (colliding) Galaxies and Active Galaxies Colliding galaxies tidal distortions, star formation, evolution (role of simulations) Active galaxies Beginnings – bright nuclei (Seyfert) Quasar discovery - the, high redshift surprise “Non-thermal” radiation (synchrotron +) Models: supermassive black hole + accretion Beyond the nucleus – radio galaxies & jets Superluminal motion, blazars “Unified” theories

COLLIDING GALAXIES Galaxies in collision/interacting/mergers The “Antennae” Computer simulation – interacting pair

COLLIDING GALAXIES Galaxies in collision/interacting/mergers The “Antennae” Computer simulation – interacting pair

COLLIDING GALAXIES M 51 – the Whirlpool and companion

COLLIDING GALAXIES M 51 – the Whirlpool and companion

COLLIDING GALAXIES Evidence for mergers Distant Galaxies (large lookback times) – forming via mergers

COLLIDING GALAXIES Evidence for mergers Distant Galaxies (large lookback times) – forming via mergers Ring of active star formation

COLLIDING GALAXIES Sgr dwarf elliptical merging with Milky Way

COLLIDING GALAXIES Sgr dwarf elliptical merging with Milky Way

Seyfert galaxies – spirals with very luminous central nucleus strong infrared and radio sources

Seyfert galaxies – spirals with very luminous central nucleus strong infrared and radio sources Strong emission H, He, N, O Doppler broadened lines Carl Seyfert

In 1962, British radio astronomer IDENTIFYING THE OPTICAL COUNTERPART Cyril Hazard used moon as

In 1962, British radio astronomer IDENTIFYING THE OPTICAL COUNTERPART Cyril Hazard used moon as an occultive shield RADIO XRAY OPTICAL

3 C 273 spectrum Martin Schmidt 7 x 1044 ergs/s !

3 C 273 spectrum Martin Schmidt 7 x 1044 ergs/s !

Quasars – Quasi-stellar Object (QSOs) Central source so luminous appears star-like Radio/Optical/UV/Xray/Gamma-ray radiation

Quasars – Quasi-stellar Object (QSOs) Central source so luminous appears star-like Radio/Optical/UV/Xray/Gamma-ray radiation

Giant elliptical M 87 Cen A – radio emission M 87 – jet from

Giant elliptical M 87 Cen A – radio emission M 87 – jet from nucleus

Active Galaxies Strong radio sources Radio galaxies -- jets of nonthermal radiation – two-lobed

Active Galaxies Strong radio sources Radio galaxies -- jets of nonthermal radiation – two-lobed appearance due ejection at high energies

Current work: Ph. D student Shea Brown Coma cluster of galaxies and radio “relic”

Current work: Ph. D student Shea Brown Coma cluster of galaxies and radio “relic” from infall of galaxies into cluster Blue – radio WSRT Red – X-rays ROSAT Green – diffuse radio, GBT

The central engine for active galaxies, radio galaxies, quasars -supermassive black holes 109 x

The central engine for active galaxies, radio galaxies, quasars -supermassive black holes 109 x mass Sun Our galactic center 106 x mass Sun http: //www. mpe. mpg. de/ir/GC/index. php

VLBI

VLBI

“Superluminal” motion Relativistic almost along line of sight

“Superluminal” motion Relativistic almost along line of sight

UNIFIED MODELS Radio galaxy Seyfert galaxies/ Quasars Blazars

UNIFIED MODELS Radio galaxy Seyfert galaxies/ Quasars Blazars