QSO’s The First Symposium. Background ä USAF Pilot (retired) ä “Top Secret” - “SCI” ä Worked On: ä Nuclear Weapons ä Overhead Reconnaissance ä Intelligence.

Slides:



Advertisements
Similar presentations
White Dwarf Stars Low mass stars are unable to reach high enough temperatures to ignite elements heavier than carbon in their core become white dwarfs.
Advertisements

© 2010 Pearson Education, Inc. Chapter 18 The Bizarre Stellar Graveyard.
Supernovae and nucleosynthesis of elements > Fe Death of low-mass star: White Dwarf White dwarfs are the remaining cores once fusion stops Electron degeneracy.
Copyright © 2009 Pearson Education, Inc. Chapter 13 The Bizarre Stellar Graveyard.
End States Read Your Textbook: Foundations of Astronomy
Chapter 12 Space Exploration.
Stellar Deaths II Neutron Stars and Black Holes 17.
Neutron Stars and Black Holes Please press “1” to test your transmitter.
Neutron Stars and Black Holes
Charles Hakes Fort Lewis College1. Charles Hakes Fort Lewis College2.
Active Galactic Nuclei Chapter 28 Revised Active Galactic Nuclei Come in several varieties; Starburst Nuclei – Nearby normal galaxies with unusually.
Class 18 : Stellar evolution, Part II Evolution of a 50 M  star… Black holes. Hypernovae. Gamma-Ray Bursts (GRBs)… Observational characteristics of GRBs.
AST101 The Evolution of Galaxies. Virgo Cluster Collisions of Galaxies Outside of Clusters (the field), most galaxies are spiral or irregular In dense.
Galaxies Types Dark Matter Active Galaxies Galaxy Clusters & Gravitational Lensing.
Chapter 25: Quasars and active galaxies Features of quasars Quasars and distant galaxies Seyfert and radio galaxies Active galactic nuclei Supermassive.
Chapter 10 – part 3 - Neutron stars and Black Holes Neutron stars.
Nebulas are made up of gas left behind by stars forming or exploding There are different classes of Nebulas The classes are: Reflection Nebulae, Emission.
The Discovery of Quasars (the first AGN found) Maartin Schmidt – the ‘discoverer of quasars’ Cyril Hazard – the REAL DEAL.
Galaxies Chapter 13:. Galaxies Contain a few thousand to tens of billions of stars, Large variety of shapes and sizes Star systems like our Milky Way.
Black holes: do they exist?
Do black holes really exist? Dr Marek Kukula, Royal Observatory Greenwich.
Stars, Galaxies, and the Universe.  To understand how telescopes work, its useful to understand the nature of the electromagnetic radiation. Light is.
This is the Local Group of galaxies, about 45 galaxies within about 1 Mpc of the Milky Way. Most are dwarf-elliptical or iregular. A distance of one million.
Stars.
Star Properties. Where do stars come from? Stars form in a cloud of dust and gas in space called a nebula.
Black Hole (BH)  Introduction to BH  Motivation to study BH  Formation of BH  Cool slides  Size of BH  Properties of BH  Evidence for BH.
Remnant of a Type II supernova explosion Iron core collapses until neutrons are squeezed tightly together During the explosion core remains intact, outer.
Starbursts, Interacting Galaxies and Active Galactic Nuclei (AGNs) Evidence for close encounters, collisions & mergers Eruptions and explosions -- radio.
10/15/2012 Alec Fisher QUASARS (QUASI-STELLAR RADIO SOURCES)
Black Holes This one’s green. I like green.. What happens after a SN? Material remaining after a supernova is 3 times more massive than the sun or more.
Quasars Chapter 17. Topics Quasars –characteristics –what are they? –what is their energy source? –where are they? –how old are they? –interactions of.
Death of Stars III Physics 113 Goderya Chapter(s): 14 Learning Outcomes:
ASTR 113 – 003 Spring 2006 Lecture 11 April 12, 2006 Review (Ch4-5): the Foundation Galaxy (Ch 25-27) Cosmology (Ch28-29) Introduction To Modern Astronomy.
By Katy O’Donohue. Black Holes Black Holes are a region of space from which nothing can escape, including light. Light is made up of massless particles.
Black Holes Chapter 14. Review What is the life cycle of a low mass star (
Galaxies with Active Nuclei Chapter 14:. Active Galaxies Galaxies with extremely violent energy release in their nuclei (pl. of nucleus).  “active galactic.
Earth & Space Science March 2015
Quasars and Active Galactic Nuclei
Astrophysics from Space Lecture 6: Supermassive black holes Prof. Dr. M. Baes (UGent) Prof. Dr. C. Waelkens (KUL) Academic year
Quasars and Other Active Galaxies
Goal: To understand the most energetic stars in the universe, quasars Objectives: 1)To understand Quasars.
Active Galactic Nuclei Chapter 26 Revised Active Galactic Nuclei Come in several varieties; Starburst Nuclei – Nearby normal galaxies with unusually.
Ethan Fukuda Cody Tamura Period 1
It was discovered in the early 1990’s that the pulse period of a millisecond pulsar 500 parsecs from earth varies in a regular way.
PowerPoint made by Sana Gill BLACK HOLES. WHAT IS A BLACK HOLE? A black hole is an area in space-time so compact that no matter, not even light can escape.
Chapter 13 Neutron Stars and Black Holes. Optical, Infrared and X-ray Image of Cassiopeia A.
Neutron Stars & Black Holes. Neutron Stars and Black Holes I. Neutron Stars A. Remnant from the collapse of a _________. B. During the core collapse of.
Active Galaxies Galaxies with extremely violent energy release in their nuclei (pl. of nucleus). → “Active Galactic Nuclei” (= AGN) Up to many thousand.
Starbursts, Interacting Galaxies and Active Galactic Nuclei (AGNs) Evidence for close encounters, collisions & mergers Eruptions and explosions -- radio.
Galaxies. The Hubble Tuning-Fork Diagram This is the traditional scheme for classifying galaxies:
Unit 2 - Cosmology Part 1: Stars Part 2: Galaxies Part 3: Origin and Evolution of the Universe.
© 2010 Pearson Education, Inc. The Bizarre Stellar Graveyard.
Deep Space Objects Variable stars Caused by pulsations in the stars – expansions make them cooler and dimmer – Contractions make them hotter and brighter.
Stellar Evolution Continued…. White Dwarfs Most of the fuel for fusion is used up Giant collapses because core can’t support weight of outer layers any.
Supernova explosions. The lives of stars Type I supernovae –Destruction of white dwarfs Type II supernovae –Core collapse of massive stars What’s left.
Galaxies with Active Nuclei
Stars on and off the Main Sequence
Black Holes By Katy O’Donohue.
Announcements Grades for third exam are now available on WebCT
This one’s green. I like green.
Black holes, neutron stars and binary star systems
Stellar Evolution.
Quasars, Active Galaxies, and super-massive black holes
White Dwarf Stars Low mass stars are unable to reach high enough temperatures to ignite elements heavier than carbon in their core become white dwarfs.
Supernova in images of Greg Thorne and Nick McCaw
The Death of a Star.
Quasars and Active Galactic Nuclei
Quasars By Ava Pickel.
Black Holes Chapter 14.
The Death of a Star.
Presentation transcript:

QSO’s The First Symposium

Background ä USAF Pilot (retired) ä “Top Secret” - “SCI” ä Worked On: ä Nuclear Weapons ä Overhead Reconnaissance ä Intelligence ä Electronic Warfare ä Flown and Worked in: “Area 51”

Grasslands Observatory 651 Sabino Canyon Observatory 854

Nomenclature ä Quasi-Stellar Radio Sources (1963) ä Newly Discovered “Radio Sources” ä “Quasars” coined by H. Chiu at Conference ä Quasi-Stellar Objects – “QSO” ä 1969 ä All Objects (Radio-Loud and Radio-Quiet (99%))

My Interest in Astrophysics Began: 16 December 1963

First Texas Symposium on Relativistic Astrophysics

International Symposium on Gravitational Collapse and other topics in Relativistic Astrophysics December 1963

Agenda

My First Symposium ä I Sat for Three Days: ä Between: ä F. Hoyle and W. Fowler ä Behind : ä M. Schmidt and J. A. Wheeler

HoyleFowler andMe

3C 273 “The First”

3C273

The Dallas Newspaper

Chronology of Compact Objects ä White Dwarf ä 1910 – Faintness – H. R. Russell and E. C. Pickering ä 1922 – Term Coined by W. Luyten ä 1922 – Generally Accepted ä Neutron Star ä 1934 – Proposed and Coined – W. Baade and F. Zwicky ä 1963 – “Cut Off Gravitationally” from Detection ä 1967 – Discovery of M1 Pulsar – J. Bell and A. Hewish ä 1967 – Generally Accepted

Chronology of Compact Objects ä Black Hole ä 1915 – Proposed – K. Schwarzschild ä 1939 – Mass and Singularity ä J. R. Oppenheimer, H. Snyder and G.M. Volkoff ä 1963 – Rotating Black Holes – R. Kerr ä 1967 – Term Coined – J. Wheeler ä “Frozen Stars” ä 1969 – QSO’s were Supermassive Black Holes ä D. Lynden-Bell ä 1974 – Accretion Disk – D. Lynden-Bell ä 1975 ? – Generally Accepted

Before “The Symposium” ä 1960 Discovery ä 1 st “Radio Star” – 3C 48 by A.Sandage ä 48 th Source in the 3 rd Cambridge Catalogue ä Variable so must be “Stellar” (Strange Spectrum) ä 1962 Discovery ä 3C 273 Occultation by C. Hazard ä December Spectrum by M. Schmidt ä Recognized Lines in March 1963

Known Quasars (December 1963) ä 3C 48 – Mag = – z = ä 3C 147 – Mag = – z = ä 3C 196 – Mag = – z = ä 3C 273 – Mag = – z = ä 3C 286 – Mag = – z = ( Galaxy 3C z= 0.46 )

This Symposium ä 300 of Brightest Astronomers and Astrophysicists ä Wrestling with the New Data on “Quasars” ä Looking for a “New” Ideas/Theories ä Give and Take – Became a Debate of Ideas ä Challenges to Each New Idea ä Many “Wild Ideas” Were Proposed ä Kick Started a Paradigm Shift in Thinking

Symposium ä Unheard of Distances – 2 to 9 Billion Light Years ä 50 Times the Luminosity of Brightest Galaxy ä Very Small – A Few Light Months Across ä The Question – What is The Energy Source? ä Supernova Chain Reactions (G. Burbidge) ä Collision of a Galaxy and a Anti-Galaxy ä Condensation of One Million White Dwarfs ä Gravitational Collapse of Superstar (Hoyle and Fowler) ä Gravitational Energy Release (Hoyle and Fowler)

Features of Quasars ä Massive Objects ≥ 10 8 Solar Mass ä Less Than One Parsec Across ä Are a Coherent Mass (not Stars) ä Lifetimes of at Least 10 6 Years ä Variations in Optical of ~ 30%/year ä Radiate in Radio, More Strongly in Optical ä Tenuous Matter ä Particle-Number Density of the Order of 10 7 /cm 3 ä Total Energy ≥ 10 6 Solar Mass

Discussion ä Discussed ä Compact Objects ä White Dwarfs ä Superstars – 10 6 to 10 9 Solar Mass ä Singularities ä (Schwarzschild) ä Implosion ä Gravitational Collapse ä Gravitational Energy Released to ergs ä Not Discussed ä Accretion Disks ä Event Horizon ä Black Holes

Hoyle’s Ideas

11 March 1966

Quasi-Poem Twinkle, Twinkle, Quasi-Star Biggest puzzle from afar How unlike the other ones Brighter than a billion suns Twinkle, Twinkle, Quasi-Star How I wonder what you are. George Gamow

“Heaven’s New Enigma” ä A Most Memorable Experience ä Life long interest in QSO’s ä From 3C 273 to …..

3C273

Visual Observation 23 December 1963

“We have encountered a most baffling group of astronomical objects. Whether fundamental new processes lie behind their brilliant but ephemeral appearance, or whether our imaginations are still too limited remains for the future to determine.” Jesse L. Greenstein

QSO’s ä Total = 117,792 ä Most Distant ä J – z = ä Most Luminous ä Ultraluminous BAL QSO APM ä 5 x L (~ 25,000 Milky Way’s)

Questions

3C 273

Redshift Z (Redshift) Light Travel Time (Gyr) Comoving Radial Distance (Gly) ~ 2X 6.42 * ~ 3X