Quasars.

Slides:



Advertisements
Similar presentations
February 9, 11:00 am. The unusually bright centers found in some galaxies are called 1.active galactic nuclei. 2.starbursts. 3.halos. 4.supermassive.
Advertisements

Slide 1 Andromeda galaxy M31Milky Way galaxy similar to M31.
AST101 The Evolution of Galaxies. Virgo Cluster Collisions of Galaxies Outside of Clusters (the field), most galaxies are spiral or irregular In dense.
QUASARS Monsters of the ancient Universe Professor Jill Bechtold Steward Observatory Tucson Amateur Astronomers, Dec. 6, 2002.
© 2010 Pearson Education, Inc. Chapter 21 Galaxy Evolution.
Galaxies Types Dark Matter Active Galaxies Galaxy Clusters & Gravitational Lensing.
Class 24 : Supermassive black holes Recap: What is a black hole? Case studies: M87. M106. MCG What’s at the center of the Milky Way? The demographics.
Chapter 25: Quasars and active galaxies Features of quasars Quasars and distant galaxies Seyfert and radio galaxies Active galactic nuclei Supermassive.
ASTR100 (Spring 2008) Introduction to Astronomy Galaxy Evolution & AGN Prof. D.C. Richardson Sections
Galaxies and the Foundation of Modern Cosmology III.
Lecture 9: Quasars & “Active” Galaxies Astronomy 5: The Formation and Evolution of the Universe Sandra M. Faber Spring Quarter 2007 UC Santa Cruz.
Galaxies Chapter 16. Galaxies Star systems like our Milky Way Contain a few thousand to tens of billions of stars. Large variety of shapes and sizes.
Quasars and Other Active Galaxies
Galaxies Live in Clusters Hickson Fornax. Coma Virgo.
 Galaxies with extremely violent energy release in their nuclei  Active Galactic Nuclei (AGN)  Up to many thousand times more luminous than the entire.
Cosmology and QSO’s Edwin Hubble Red Shift and Distance 24 Mpc1200 km/s 300 Mpc15,000 km/s 780 Mpc39,000 km/s 1220 Mpc61,000 km/s.
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.
Our goals for learning How did Hubble prove galaxies lie beyond our galaxy? How do we observe the life histories of galaxies? How did galaxies form? Why.
Galaxies.
Systems containing millions, or even billions, of stars Observable universe contains as many as 50 billion to 100 billion galaxies; millions of light years.
Quasars, black holes and galaxy evolution Clive Tadhunter University of Sheffield 3C273.
Astronomy Topic 4 Revision Booster. Milky way facts 200 billion stars 250 million years to orbit One of a group of about 30 galaxies (The local group)
Lecture 40 Galaxies (continued). Evolution of the Universe. Characteristics of different galaxies Redshifts Unusual Galaxies Chapter 18.6  18.9.
© 2010 Pearson Education, Inc. Chapter 21 Galaxy Evolution.
Quasars Chapter 17. Topics Quasars –characteristics –what are they? –what is their energy source? –where are they? –how old are they? –interactions of.
January 2nd 2013 Objective Warm-Up
Galactic Nucleus. Mass of the Galaxy The orbit of clusters can be used to estimate the mass of the galaxy. –Same used for planets and binary stars The.
Galaxies with Active Nuclei Chapter 14:. Active Galaxies Galaxies with extremely violent energy release in their nuclei (pl. of nucleus).  “active galactic.
Quasars and Active Galactic Nuclei
Active Galaxies and Supermassive Black Holes Chapter 17.
Quasars and Other Active Galaxies
Quasars, Active Galaxies, and Gamma-Ray Bursters Chapter Twenty-Seven.
Chapter 21 Galaxy Evolution Looking Back Through Time Our goals for learning How do we observe the life histories of galaxies? How did galaxies.
Dec 3, 2003Astronomy 100 Fall 2003 Homework due on Friday– 11:50 am Honor credit– need to have those papers soon! THE FINAL IS DECEMBER 15 th : 7-10pm!
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.
Universe Tenth Edition Chapter 24 Quasars and Active Galaxies Roger Freedman Robert Geller William Kaufmann III.
A single galaxy with its millions or billions of stars is only a very small spot in the observable universe. Galaxies & AGN’s (Chapter 13) Hercules Cluster.
Galaxies with Active Nuclei
Galaxies.
Galaxies and the Universe
Announcements Grades for third exam are now available on WebCT
© 2017 Pearson Education, Inc.
Evolution of Black Hole Masses from Spectra of Quasar Gas Dynamics
Quasars and Active Galaxies
Stars, Galaxies, and the Universe
Peculiar (colliding) Galaxies and Active Galaxies
Question of the Day What determines the path of the life cycle for a star? WWBAT: Describe the three types of galaxies Size.
Ch.1, Sec.2 - Telescopes Optical Telescopes
Objectives Describe how astronomers classify galaxies.
Section 2: Other Galaxies in the Universe
Quasars, Active Galaxies, and super-massive black holes
Galaxies and the Universe
Using Telescopes to Observe Electromagnetic Radiation in Space
THE UNIVERSE What would we see if we were to look deep into a very black part of the sky at night?
ASTR 1040 – November 30 Planetarium, December 5
Chapter 21 Galaxy Evolution
© 2017 Pearson Education, Inc.
Chapter 21 Galaxy Evolution and Black Holes
Galaxies.
Active Galaxies.
Quasars and Active Galactic Nuclei
Note that the following lectures include animations and PowerPoint effects such as fly ins and transitions that require you to be in PowerPoint's Slide.
Galaxies With Active Nuclei
NOTES: Active Galactic Nuclei (AGN)
But first dwarf and other special galaxies
Galaxies With Active Nuclei
Milky Way and other Galaxies
Giant Elliptical Galaxies
Structure, Types, Known Galaxies
Presentation transcript:

Quasars

Distant Light Some objects in deep space are visible, small, and have large redshifts. Very distant by Hubble’s law Billions of light years away larger wavelength nearby galaxy distant object

Quasi-Stellar Objects These objects were first observed as intense radio sources. Bright, but star-sized They were named quasi-stellar radio sources—quasars. Quasars emit in all parts of the electromagnetic spectrum. 100 times Andromeda Brighter flares 3C279, a quasar photographed in gamma rays

Distant Past Looking at a faraway object is like looking back in time. If a quasar is 4 billion ly away, we are seeing the universe 4 billion years ago. Early life of galaxies Andromeda — 2 million years ago Earth PKS 1127 — 4 billion years ago

Disk and Jets Radio measurements show two giant jets of radiating gas. Visible light and x-rays see a disk of gas, dust and stars. Most intense at center

Jet Formation Quasars form from a supermassive black hole. The black hole draws stars and dust to its center. The material is accelerated to high velocity and ejected out either side.

Active Nuclei Some nearby galaxies show jets of radiating gas. Start at galactic black hole Active from dust falling in Quasars fade to active galaxies as dust decreases.

Radio Galaxies Visible elliptical galaxies have black holes in their center. The jets are only seen with radio telescopes. Radio galaxies Active spiral galaxies are called Seyfert galaxies.

Colliding Black Holes The Chandra X-ray Observatory has observed two supermassive black holes in the same galaxy. NGC 6240: 400 Mly When the holes collide in a few hundred million years, the gravity waves will be felt on earth.