ASP2011 Measurement Techniques Lectures 7-8 Dr. Duncan Galloway University of Melbourne

Slides:



Advertisements
Similar presentations
High energy Astrophysics Mat Page Mullard Space Science Lab, UCL Revision lecture.
Advertisements

ATHENA: The Advanced Telescope for High Energy Astrophysics
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.
Chandra X-ray Observatory Your Name Title Date CHANDRA X-RAY OBSERVATORY Presentation to X.
1 Stellar Remnants White Dwarfs, Neutron Stars & Black Holes These objects normally emit light only due to their very high temperatures. Normally nuclear.
YSS - Intro. to Observational Astrophysics (ASTR 205). Class #10 The Bizarre Stellar Graveyard (Chapter 13) Professor: José Maza June 20, 2011 Professor:
9 v 2012Kavli IPMU1 Computational Astrophysics at the Kavli Institute for Particle Astrophysics and Cosmology at Stanford Roger Blandford.
Neutron Star Spins Down 0 Topic: Neutron stars Concepts: Pulsars, magnetic fields, pulsar timing Missions: Swift, Fermi Coordinated by the NASA Astrophysics.
Mass transfer in a binary system
Binary Stellar Evolution How Stars are Arranged When stars form, common for two or more to end up in orbit Multiples more common than singles Binaries.
ASTR 113 – 003 Spring 2006 Lecture 07 March 8, 2006 Review (Ch4-5): the Foundation Galaxy (Ch 25-27) Cosmology (Ch28-39) Introduction To Modern Astronomy.
LECTURE 20, NOVEMBER 9, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT 1ASTR 101-3, FALL 2010.
Neutron Stars Chapter Twenty-Three.
Vicky Kaspi McGill University Lorne Trottier Chair in Astrophysics and Cosmology.
A Galaxy Revealed in Multiple Wavelengths 0 Topic: Multiwavelength observations Concepts: Infrared observations, X-ray observations, Optical observations,
Earth Science 25.2B : Stellar Evolution
X Ray Astronomy Presented by:- Mohit Shashwat Ankit.
LIGO-G W What If We Could Listen to the Stars? Fred Raab LIGO Hanford Observatory.
Laser Interferometer Gravitational-Wave Observatory Who? Presented By: Bonnie Wooley.
China’s Future Missions in Space High Energy Astrophysics Shuang Nan Zhang 张双南 Tsinghua University and Institute of High Energy Physics, Chinese Academy.
GALAXY FORMATION AND EVOLUTION - 2. DISCOVER Magazine’s 2007 Scientist of the Year David Charbonneau, of the Harvard-Smithsonian Canter for Astrophysics.
Gravitational-waves: Sources and detection
Compact Objects Astronomy 315 Professor Lee Carkner Lecture 15 “How will we see when the sun goes dark?” “We will be forced to grope and feel our way.”
The Life Cycle of a Star Presenters:. The Life Cycle of a Low-Mass Star Stellar Nebula Giant White Dwarf.
A body of matter Vague and Indistinct shape Dense mass No amount of light can break out Black Hole, Gravitational Force and Mass.
Quasars and Other Active Galaxies
Teória relativity začiatok alebo koniec fyziky.
Black holes: do they exist?
Nearby Galaxy Evolution Prof. Gerhardt R Meurer. Galaxy evolution in a nutshell Galaxy Evolution2  Time machines  The farther we peer  The farther.
Big Bang Theory Created by Evan Chernenko Click to Start.
Space Exploration- Tools
NASA and us Ms. Wood. Things you should know Moon revolves around sun as it revolves around Earth Millions of galaxies Solar system is made of: Sun Planets.
1 Stellar Remnants White Dwarfs, Neutron Stars & Black Holes These objects normally emit light only due to their very high temperatures. Normally nuclear.
Wikipedia Commons  Einstein views Gravity NOT as a force, but as a bending of spacetime  It still affects how things move, but not as an attractive.
Death of large stars Chapter 21&22 Supernova Ia Death of high mass stars: Neutron stars Pulsars Black holes.
Nobel Prize in Physics: Riccardo Giacconi. Short Bio Born in Italy, Riccardo Giacconi earned his Ph.D. in cosmic ray physics at the University of Milan.
ASTR 567: Observational Techniques in Astronomy. ASTR 567: Grading Scheme Start of lecture quizzes………………….. 10% Homeworks……………………………………..25% Highest of.
A multiwavelength approach is needed to discover a quasars’ behaviour as a whole and uncover its structure. This means obtaining data from the long wavelength.
Black Holes. Black holes The gravity on neutron stars, white dwarfs and black dwarfs is so strong that it crushes atoms, so the matter in stars is millions.
Stellar Evolution. Solar Composition Most stars in space have this composition: 74% hydrogen, 26% helium Fusion is the energy maker of the sun.
Galaxies with Active Nuclei Chapter 14:. Active Galaxies Galaxies with extremely violent energy release in their nuclei (pl. of nucleus).  “active galactic.
YSS - Intro. to Observational Astrophysics (ASTR 205). Class #10 The Bizarre Stellar Graveyard (Chapter 13) Professor: José Maza July 3, 2012 Professor:
Earth & Space Science March 2015
W. Udo Schröder, 2007 Applications Applications of Nuclear Instruments and Methods 1.
Quasars and Other Active Galaxies
What is Astronomy? An overview..
Small Satellite Conference - GEMS Presentation August 12, 2009 Big Astrophysics in A Small Package Erin Walter GEMS Spacecraft Lead/Orbital.
The Search for Black Holes
Birth and Death of Stars. Astronomers learn about stars by observing the electromagnetic radiation the stars emit. The most common type of telescope collects.
LIGO-G Z1 Using Condor for Large Scale Data Analysis within the LIGO Scientific Collaboration Duncan Brown California Institute of Technology.
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.
High energy Astrophysics Mat Page Mullard Space Science Lab, UCL 1. Overview.
October 17, 2003Globular Clusters and Gravitational Waves1 Gravitational Wave Observations of Globular Clusters M. Benacquista Montana State University-Billings.
Copyright © 2010 Pearson Education, Inc. Clicker Questions Chapter 13 Neutron Stars and Black Holes.
The Search for Black Holes
Astronomy: A Beginner’s Guide to the Universe Seventh Edition © 2013 Pearson Education, Inc. Neutron Stars and Black Holes Chapter 13 Clickers.
A101 Slide Set: Shockingly Bright Pulsar Developed by the NuSTAR EPO Group at Sonoma State University 0 Topic: Pulsars, X-rays, black holes Concepts: multi-wavelength.
HOW TO DETECT A BLACK HOLE Effects on matter/light outside the horizon –gravitational attraction of other bodies –“dark star” with mass distinguish from.
Astro 101 Slide Set: Binary System Makes Near Miss Developed by the WISE team 0 Topic: Close pass of binary system Concepts: Solar neighborhood, red dwarfs,
Gamma-Ray Bursts Please press “1” to test your transmitter.
Lives of Stars.
Nergis Mavalvala (age 47)
A Galaxy Revealed in Multiple Wavelengths
What is Astronomy? An overview..
The Laser Interferometer Gravitational-Wave Observatory
What is Astronomy? An overview..
The Death of a Star.
The Death of a Star.
What is Astronomy? An overview..
ASTR Fall Semester [Slides from Lecture17]
Presentation transcript:

ASP2011 Measurement Techniques Lectures 7-8 Dr. Duncan Galloway University of Melbourne

Cover of the UCSD phonebook, 1995 Caption reads: “Pictured on the cover is Dr. Richard Rothschild with one of the clusters of X-ray detector instruments designed, fabricated and tested at UCSD's Center for Astrophysics & Space Sciences for NASA's X-ray Timing Explorer. The instrument, along with others developed at the Massachusetts Institute of Technology and NASA's Goddard Space Flight Center, will provide important information on the nature of X- ray emitting objects, such as black holes, neutron stars, and white dwarfs. The products of stellar evolution, these extremeley dense objects exhibit enormous gravitational fields and are ultimately responsible for the generation of X-rays and gamma rays. Scheduled for launch in August 1995, the X-ray Timing Explorer will exploit the temporal variability of these stars on time scales from millionths of a second to months to explain how matter is transferred from one star to its binary companion, how this matter interacts with the intense magnetic fields present, and how X-ray beams are formed. The mission will also provide scientists with new understanding of the dynamics and life history of X-ray emitting objects.

LIGO Hanford, Washington LIGO Livingston, Louisiana

Standard telescope setup Modifications for adaptive optics