The Galactic Centre: a hidden treasure How can we study the Galactic centre? How can we study the Galactic centre? What is do we find there? What is do.

Slides:



Advertisements
Similar presentations
Chapter 15: The Milky Way Galaxy
Advertisements

LECTURE 21, NOVEMBER 16, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT 1ASTR 101-3, FALL 2010.
Chapter 21: The Milky Way. William Herschel’s map of the Milky Way based on star counts In the early 1800’s William Herschel, the man who discovered the.
Introduction to Astrophysics Lecture 13: The Milky Way Galaxy.
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.
Slide 1 Andromeda galaxy M31Milky Way galaxy similar to M31.
Chapter 15 The Milky Way Galaxy.
14.2 Galactic Recycling Our Goals for Learning How does our galaxy recycle gas into stars? Where do stars tend to form in our galaxy?
A105 Stars and Galaxies  Milky Way Homework (#11) due today  Projects Due Nov. 30  For next week: Units 74, 75, 76, 78, 79  “rooftop” tonight, 8 PM,
The Milky Way Galaxy Chapter 15. The Milky Way Almost everything we see in the night sky belongs to the Milky Way We see most of the Milky Way as a faint.
The Milky Way Galaxy part 2
QUASARS Monsters of the ancient Universe Professor Jill Bechtold Steward Observatory Tucson Amateur Astronomers, Dec. 6, 2002.
The Milky Way PHYS390 Astrophysics Professor Lee Carkner Lecture 19.
15 The Milky Way More than just a candy bar.. 15.
Chapter 15 The Milky Way Galaxy.
The Mass of the Galaxy We can use the orbital velocity to deduce the mass of the Galaxy (interior to our orbit): v orb 2 =GM/R. This comes out about 10.
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.
At the Center of the Galaxy!. Galaxy Centers are Mysterious and Wild Below is a picture of where the Galaxy center is with respect to the horizon (for.
9B The Milky Way Our Galactic Home. 9B 9B Goals Structure of our Galaxy. Its size and shape. How do stars and things move through it? Mass and Dark Matter.
The Milky Way Center, Shape Globular cluster system
Caty Pilachowski Mini-University 2013 Our Milky Way in Space and Time.
The Milky Way Galaxy Immanuel Kant (1724 – 1804) German philosopher The infinitude of creation is great enough to make a world, or a Milky Way of worlds,
Levels of organization: Stellar Systems Stellar Clusters Galaxies Galaxy Clusters Galaxy Superclusters The Universe Everyone should know where they live:
The Milky Way Galaxy.
Our Galaxy The Milky Way. The Milky Way Almost everything we see in the night sky belongs to the Milky Way We see most of the Milky Way as a faint band.
The Milky Way Our Galaxy Please press “1” to test your transmitter.
The Milky Way Galaxy Chapter 12:. The Milky Way Almost everything we see in the night sky belongs to the Milky Way. We see most of the Milky Way as a.
The Milky Way and Other Galaxies Science A-36 12/4/2007.
What’s Brewing in the Teapot? M7 M6 M8 M22 Caty Pilachowski IU Astronomy.
Black holes: do they exist?
 Galaxies with extremely violent energy release in their nuclei  Active Galactic Nuclei (AGN)  Up to many thousand times more luminous than the entire.
Galaxies.
The Milky Way Galaxy.
Quasars, black holes and galaxy evolution Clive Tadhunter University of Sheffield 3C273.
Galaxy Collisions Top left is an image of the Cartwheel galaxy. The ring of young stars was likely created as a smaller galaxy passed through the disk.
Susan CartwrightOur Evolving Universe1 The Milky Way n From a dark site the Milky Way can be seen as a broad band across the sky l l What is it?   telescopes.
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.
Introduction to Galaxies 5/23/2013. BR: Milky Way Scale The Milky Way has a diameter of approximately 8.25 x 10 9 AU (8.25 billion AU). 206,265 AU = 3.26.
ASTR112 The Galaxy Lecture 7 Prof. John Hearnshaw 11. The galactic nucleus and central bulge 11.1 Infrared observations (cont.) 11.2 Radio observations.
1 The Milky Way Galaxy We live on the quiet outskirts of a galaxy of approximately 100 Billion stars. This galaxy, the Milky Way, is roughly disk-shaped.
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
Active Galaxies and Supermassive Black Holes Chapter 17.
The Milky Way Galaxy. Sky Maps in Different Bands.
UNIT 1 The Milky Way Galaxy.
AST101 Lecture 19 Discovery of the Galaxy. Northern Milky Way.
Copyright © 2010 Pearson Education, Inc. Clicker Questions Chapter 14 The Milky Way Galaxy.
Our Milky Way Galaxy. The Milky Way Almost everything we see in the night sky belongs to the Milky Way. We see most of the Milky Way as a faint band of.
Copyright © 2010 Pearson Education, Inc. Chapter 14 The Milky Way Galaxy Lecture Outline.
Galaxies: Our Galaxy: the Milky Way. . The Structure of the Milky Way Galactic Plane Galactic Center The actual structure of our Milky Way is very hard.
A Long Time Ago in a Galaxy Far, Far Away…. The Milky Way Galaxy: Home Sweet Home!! Our home Galaxy is called the MILKY WAY (like the candy bar ) Our.
Our Galaxy Chapter Twenty-Five. Guiding Questions 1.What is our Galaxy? How do astronomers know where we are located within it? 2.What is the shape and.
How We See Ourselves In The Universe: A Look At The Galaxies That Surround Us.
The Milky Way Galaxy This is a picture of the Sombrero Galaxy NOT The Milky Way.
Elliptical: Circular or elliptical in shape, have no gas and dust, with no visible bright stars or spiral patterns. Elliptical galaxies probably comprise.
© 2017 Pearson Education, Inc.
More than just a candy bar.
Journey to the Galactic Center
The Milky Way Galaxy.
The “Milky Way”.
Our Milky Way Galaxy.
GALAXIES!.
The Milky Way Our Galactic Home.
Galaxies.
When Giovanni Riccioli used a telescope like this one to observe a star in the handle of the Big Dipper, he discovered two stars that orbit each other.
The Milky Way Galaxy.
Galaxies.
The Milky Way Galaxy.
Dust Dust cloud The disk Lots of dust in spiral galaxies The bulge
Presentation transcript:

The Galactic Centre: a hidden treasure How can we study the Galactic centre? How can we study the Galactic centre? What is do we find there? What is do we find there? What does it tell us about our Galaxy, and galaxies in general? What does it tell us about our Galaxy, and galaxies in general?

Galactic Bulges Classic view of spiral galaxies Classic view of spiral galaxies young stars in spiral arms old stars in halo and bulge therefore, expect Galactic centre to be a quiet collection of old stars (like a globular cluster)? therefore, expect Galactic centre to be a quiet collection of old stars (like a globular cluster)?

Observing the Milky Way 75 cm 21 cm 11 cm 2.6 mm 60 μm 8 μm 2 μm optical X-ray γ-ray

The Galactic Centre: Radio central 4° square central 4° square numerous supernova remnants numerous supernova remnants so, not a quiet region of old stars! filamentary structures suggesting complicated magnetic fields filamentary structures suggesting complicated magnetic fields bright central source, Sgr A bright central source, Sgr A

Zooming In The Very Large Array, New Mexico The Very Large Array, New Mexico 27 telescopes in Mercedes star movable on rails data processed to mimic one large telescope resolution can be better than HST!

Zooming In NRAO / AUI / NSF 20 cm 6 cm 3.6 cm1.2 cm Sgr A*

The Galactic Centre: X-rays X-ray images pick up hot gas and “astrophysical par- ticle accelerators” such as pulsars and X-ray binaries radio image for comparison images from Chandra website

The Galactic Centre: X-rays radio image for comparison

The Galactic Centre: infra-red 4.5° MSX mid-infrared view (4.2 – 26 microns) showing mostly warm dust

The Galactic Centre: infra-red MPG/ESO near infrared (2 microns) shows stars

Mysteries of the Galactic Centre A region of intense star formation surrounding a point source of radio and X-ray emission A region of intense star formation surrounding a point source of radio and X-ray emission Where does the gas come from? What is the central point source?

Bringing in the Gas Evidence from star counts and extinction studies shows Milky Way is a barred spiral with a ring structure, like M95 Evidence from star counts and extinction studies shows Milky Way is a barred spiral with a ring structure, like M95 This allows gas from the disc to be drawn in towards the centre This allows gas from the disc to be drawn in towards the centre Image by Jean-Charles Cuillandre and Giovanni Anselme, CFHT

Sgr A* Stars in infra-red images are seen to move around Sgr A* Stars in infra-red images are seen to move around Sgr A* plot orbits plot orbits determine mass of Sgr A* determine mass of Sgr A* result: approximately solar masses! result: approximately 4 million solar masses!

The Milky Way’s dark heart Is Sgr A* a supermassive black hole? Is Sgr A* a supermassive black hole?  YES! How do we know? How do we know?  Basically, it’s too small to be anything else orbit of star S2 orbit of star S2 rapid flares in X-ray and near infra-red rapid flares in X-ray and near infra-red

The black hole mystery The Milky Way is not alone! The Milky Way is not alone! most large galaxies have central supermassive black holes most large galaxies have central supermassive black holes the black hole mass is closely correlated with the mass of the galaxy’s bulge the black hole mass is closely correlated with the mass of the galaxy’s bulge we don’t know why (yet) we don’t know why (yet) note that we believe these central black holes are the power sources of active galactic nuclei note that we believe these central black holes are the power sources of active galactic nuclei

Conclusions The centre of the Milky Way galaxy is an exciting place (if not an ideal holiday spot!) The centre of the Milky Way galaxy is an exciting place (if not an ideal holiday spot!) it is a site of active star formation with numerous young, massive stars and recent supernovae it is a site of active star formation with numerous young, massive stars and recent supernovae at its heart is a 3-million-solar-mass black hole at its heart is a 3-million-solar-mass black hole further studies may give new insights on galaxy formation further studies may give new insights on galaxy formation