Active Galactic Nuclei (AGNs): A type of AGNs: Quasars. Whatever is powering these QSO s must be very small!!

Similar documents
4/18/17. Our Schedule. Revisit Quasar 3C273. Dark Matter in the Universe. ASTR 1040: Stars & Galaxies

A. Thermal radiation from a massive star cluster. B. Emission lines from hot gas C. 21 cm from hydrogen D. Synchrotron radiation from a black hole

Galaxies with Active Nuclei. Active Galactic Nuclei Seyfert Galaxies Radio Galaxies Quasars Supermassive Black Holes

4/12/18. Our Schedule. Measuring big distances to galaxies. Hamilton on Hawking tonight. Brightness ~ Luminosity / (Distance) 2. Tully-Fisher Relation

Active Galactic Nuclei

Chapter 17. Active Galaxies and Supermassive Black Holes

ASTR 1040: Stars & Galaxies

Quasars: Back to the Infant Universe

Lecture 9. Quasars, Active Galaxies and AGN

Active Galaxies & Quasars

Question 1. Question 2. Correct. Chapter 16 Homework. Part A

Galaxies. Galaxy Diversity. Galaxies, AGN and Quasars. Physics 113 Goderya

Active Galactic Nuclei

Active Galaxies and Quasars

Lecture 11 Quiz 2. AGN and You. A Brief History of AGN. This week's topics

Astr 2320 Thurs. April 27, 2017 Today s Topics. Chapter 21: Active Galaxies and Quasars

ASTR 1040 Accel Astro: Stars & Galaxies

ASTR 101 General Astronomy: Stars & Galaxies

Chapter 19 Galaxies. Hubble Ultra Deep Field: Each dot is a galaxy of stars. More distant, further into the past. halo

A100H Exploring the Universe: Quasars, Dark Matter, Dark Energy. Martin D. Weinberg UMass Astronomy

Star systems like our Milky Way. Galaxies

Lecture Outlines. Chapter 24. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.

Feeding the Beast. Chris Impey (University of Arizona)

Chapter 21 Galaxy Evolution. How do we observe the life histories of galaxies?

Guiding Questions. Active Galaxies. Quasars look like stars but have huge redshifts

ASTR 101 Introduction to Astronomy: Stars & Galaxies

Part two of a year-long introduction to astrophysics:

A zoo of transient sources. (c)2017 van Putten 1

Chapter 15 The Milky Way Galaxy. The Milky Way

Quasars and Active Galactic Nuclei (AGN)

Galaxies. With a touch of cosmology

Astronomy 210 Final. Astronomy: The Big Picture. Outline

QUASARS and ACTIVE GALAXIES. - a Detective Story

The Classification of Galaxies

Chapter 15 Galaxies and the Foundation of Modern Cosmology

Black Holes & Quasars 18 Nov

(Astronomy for Dummies) remark : apparently I spent more than 1 hr giving this lecture

A Unified Model for AGN. Ryan Yamada Astro 671 March 27, 2006

2.3 Peculiar galaxies. Discovering Astronomy : Galaxies and Cosmology 17. Figure 21: Examples of colliding galaxies.

Dark Matter ASTR 2120 Sarazin. Bullet Cluster of Galaxies - Dark Matter Lab

Black Holes in Hibernation

1932: KARL JANSKY. 1935: noise is identified as coming from inner regions of Milky Way

Chapter 15 2/19/2014. Lecture Outline Hubble s Galaxy Classification. Normal and Active Galaxies Hubble s Galaxy Classification

Chapter 21 Galaxy Evolution. Agenda

Active Galaxies. Lecture Topics. Lecture 24. Active Galaxies. Potential exam topics. What powers these things? Lec. 24: Active Galaxies

Active galactic nuclei (AGN)

ASTR 101 Introduction to Astronomy: Stars & Galaxies

Black Hole Spins of Radio Sources

11/8/18. Tour of Galaxies. Our Schedule

IX. Stuff that's Bigger than the Solar System

The Milky Way Galaxy

Quasars and AGN. What are quasars and how do they differ from galaxies? What powers AGN s. Jets and outflows from QSOs and AGNs

Energy Source for Active Galactic Nuclei

Learning Objectives: Chapter 13, Part 1: Lower Main Sequence Stars. AST 2010: Chapter 13. AST 2010 Descriptive Astronomy

Tour of Galaxies. Sgr A* VLT in IR + adaptive optics. orbits. ASTR 1040 Accel Astro: Stars & Galaxies VLT IR+AO

Chapter 19 Reading Quiz Clickers. The Cosmic Perspective Seventh Edition. Our Galaxy Pearson Education, Inc.

Active Galactic Alexander David M Nuclei

The hazy band of the Milky Way is our wheel-shaped galaxy seen from within, but its size

Hubble s Law & Black Holes at a Galaxy s Center. Simplicio s questions about Hubble s Law

Extragalactic Radio Sources. Joanne M. Attridge MIT Haystack Observatory

M31 - Andromeda Galaxy M110 M32

The Neighbors Looking outward from the Sun s location in the Milky Way, we can see a variety of other galaxies:

Today in Astronomy 142: supermassive black holes in active-galaxy nuclei

Next. more on the.. ASTR 101 General Astronomy: Stars & Galaxies. Supermassive Black Holes and galaxies grow together

Supermassive Black Holes

The Milky Way: Home to Star Clusters

Galaxy Classification

Ac#ve Galaxies, Colliding Galaxies

The final is Thursday, July 2nd in class. Don t be late! The test will cover Chapters 1-16 and with a STRONG EMPHASIS on Chapters 9-16, 18, and

Astronomy 102 Lecture 17

Astronomy across the spectrum: telescopes and where we put them. Martha Haynes Discovering Dusty Galaxies July 7, 2016

Observing the Night Sky. Observing the Night Sky. Observing the Night Sky. Observing the Night Sky. Observing the Night Sky. Chapter 29 THE UNIVERSE

Black Holes and Active Galactic Nuclei

Lecture Outlines. Chapter 25. Astronomy Today 7th Edition Chaisson/McMillan Pearson Education, Inc.

Astronomical Research at the Center for Adaptive Optics. Sandra M. Faber, CfAO SACNAS Conference October 4, 2003

Probing the Origin of Supermassive Black Hole Seeds with Nearby Dwarf Galaxies. Amy Reines Einstein Fellow NRAO Charlottesville

ASTR 100. Lecture 28: Galaxy classification and lookback time

Active Galaxies & Emission Line Diagnostics

Our Solar System: A Speck in the Milky Way

Lecture 19: Galaxies. Astronomy 111

BROCK UNIVERSITY. Test 2, March 2015 Number of pages: 9 Course: ASTR 1P02 Number of Students: 420 Date of Examination: March 5, 2015

Quasars ASTR 2120 Sarazin. Quintuple Gravitational Lens Quasar

Active galaxies. Some History Classification scheme Building blocks Some important results

AST Cosmology and extragalactic astronomy. Lecture 20. Black Holes Part II

Powering Active Galaxies

Vera Genten. AGN (Active Galactic Nuclei)

2. Active Galaxies. 2.1 Taxonomy 2.2 The mass of the central engine 2.3 Models of AGNs 2.4 Quasars as cosmological probes.


1. This question is about Hubble s law. The light received from many distant galaxies is red-shifted. (a) State the cause of this red-shift (1)

Multi-wavelength Surveys for AGN & AGN Variability. Vicki Sarajedini University of Florida

Active Galactic Nuclei

It is about 100,000 ly across, 2,000 ly thick, and our solar system is located 26,000 ly away from the center of the galaxy.

Other Galaxy Types. Active Galaxies. A diagram of an active galaxy, showing the primary components. Active Galaxies

Active Galaxies and Galactic Structure Lecture 22 April 18th

Quasars are supermassive black holes, found in the centers of galaxies Mass of quasar black holes = solar masses

Today. Lookback time. ASTR 1020: Stars & Galaxies. Astronomy Picture of the day. April 2, 2008

NGC4038/4039, Antennae Galaxies

Bright Quasar 3C 273 Thierry J-L Courvoisier. Encyclopedia of Astronomy & Astrophysics P. Murdin

Galaxies. CESAR s Booklet

Chapter 25: Galaxy Clusters and the Structure of the Universe

Transcription:

Active Galactic Nuclei (AGNs): Galaxies with lots of activity AST 101 General Astronomy: Stars & Galaxies Some galaxies at high redshift (large lookback times) have extremely active centers More than 1000 times the light of the entire Milky Way combined from a point source at the center!! A type of AGNs: Quasars Quasi-Stellar Radio Source Nuclei so bright (at nearly all wavelengths) that the rest of the galaxy is not easily seen First discovered as radio sources - then found to have very large redshifts! Whatever is powering these QSO s must be very small!! Some quasars can double their brightness within a few hours. Therefore they cannot be larger than a few lighthours across (solar system size) Why? Think about the time it takes light from the front of the object to get to us compared to the light from the back.

Quasar Central Engines How do quasars emit so much light in so little space? They are powered by accretion disks around supermassive black In some quasars, huge jets of material are shot out at the poles. These jets are strong radio sources. Prototypical radio galaxy Giant elliptical galaxy NGC 5128 with dust lane (from spiral galaxy?) + Centaurus A radio source (color lobes) JET DISK Central Engine -- artist s conception Accretion disk around supermassive black hole Disk itself may or may not be obscured by dust If bright nucleus is visible, looks like a quasar, if not, then its a radio galaxy Cygnus A radio jets 400,000 ly Jet as fine thread, big lobes at end, central hot spot VLA

Radio tails: many shapes M87 elliptical with jet NGC 1265 100K ly 800 km/s 54 Mly away Active galactic nucleus beams out very narrow jet Accretion disk shows gas orbiting a 2.7 billion solar mass black hole first real proof in an active nucleus! 3C 31 2 M light years Another example of central beaming engine Disk around black hole in NGC 7052 GROUND radio active nucleus - HST 400 light year wide disk of material in core of elliptical galaxy with radio jets looks like a supermassive black hole at work! HST

Do ALL galaxies have supermassive black in their centers? Observations show that SMBHs grow together with galaxies during formation likely YES! Linked to the process of galaxy formation More quasars seen in the distant (early) universe than now Black gradually grow, but can run out of available fuel and become nearly invisible (like in our Milky Way) Clicker Question BH Activity resurrected by galaxy collisions? Many galaxies with bright nuclei show signs of being disturbed Collisions funnel material down into the black hole lurking at the core Expect more such collisions in denser early universe This may help explain why fewer quasars today Supermassive black at the center of galaxy are believed to be produced A. by the death of supermassive stars B. by mergers of many solar mass black C. during the process of galaxy formation D. soon after the creation of the universe E. by a magician :-)

Clicker Question Supermassive black at the center of galaxy are believed to be produced A. by the death of supermassive stars B. by mergers of many solar mass black C. during the process of galaxy formation D. soon after the creation of the universe E. by a magician :-) Next. more on the.. PAST of the Universe: structure formation FUTURE of the Universe: what is its fate? QUIZ #6 a) Describe the observations which revealed that the Universe is expanding. [2pt] b) Who performed the observations in a) and what type of measurements did he/she take? [2pt] c) Some elliptical galaxies display dust lanes in them. How did they get there given that ellipticals have very little dust? [2 pt] d) Where do Quasars get all their energy from? [2pt] e) How do we know that supermassive black grow together with their host galaxies? [2pt]