2000 l.y. M87 Astrophysics @ Purdue.

Slides:



Advertisements
Similar presentations
Space Science = Astronomy
Advertisements

Intro X-rays From the Sky Chandra X-ray Observatory November, 2003.
Gamma-Ray Astronomy Dana Boltuch Ph. D
The Extreme Universe of Gamma-ray Astronomy Professor Lynn Cominsky Department of Physics and Astronomy Sonoma State University.
ASTR100 (Spring 2008) Introduction to Astronomy Galaxy Evolution & AGN Prof. D.C. Richardson Sections
JD1 rationale Catherine Cesarsky, Diego Torres, Stefan Wagner.
Part 2: Formation of the Universe STARS AND GALAXIES 1.
Quasars and Other Active Galaxies
Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach.
What is Radio Astronomy? MIT Haystack Observatory This material was developed under a grant from the National Science Foundation.
1 Arecibo Synergy with GLAST (and other gamma-ray telescopes) Frontiers of Astronomy with the World’s Largest Radio Telescope 12 September 2007 Dave Thompson.
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.
High-Energy Astrophysics
1 Galaxies The Andromeda Galaxy - nearest galaxy similar to our own. Only 2 million light years away! Galaxies are clouds of millions to hundreds of billions.
Multiwavelength Astronomy What do different wavelength regimes allow astronomers to “see”?
Black Hole Chaos The Environments of the most super- massive black holes in the Universe Belinda Wilkes, Chandra X-ray Center, CfA Francesca Civano, CfA.
Supermassive Black Holes at the Centers of Galaxies Singles and Pairs using X-rays to study black holes disruption of stars by massive black holes pairs.
ASTR 567: Observational Techniques in Astronomy. ASTR 567: Grading Scheme Start of lecture quizzes………………….. 10% Homeworks……………………………………..25% Highest of.
Discovery of  rays from Star-Forming Galaxies New class of nonthermal sources/gamma-ray galaxies (concept of temperature breaks down at high energies)
Presented by Ellen Holmes. Hubble Space Telescope Launched August 25th, 1997  Optical telescopes gather visible light, just like our eyes, but greatly.
Earth & Space Science March 2015
Active Galaxies and Supermassive Black Holes Chapter 17.
9 May 2013: New Moon Image: May 2012 annular eclipse, Monument Valley AZ.
Gamma-Ray Bursts. Short (sub-second to minutes) flashes of gamma- rays, for ~ 30 years not associated with any counterparts in other wavelength bands.
FIRST LIGHT A selection of future facilities relevant to the formation and evolution of galaxies Wavelength Sensitivity Spatial resolution.
Chapter 21 Galaxy Evolution Looking Back Through Time Our goals for learning How do we observe the life histories of galaxies? How did galaxies.
A black hole: The ultimate space-time warp Ch. 5.4 A black hole is an accumulation of mass so dense that nothing can escape its gravitational force, not.
Active Galaxies Galaxies with extremely violent energy release in their nuclei (pl. of nucleus). → “Active Galactic Nuclei” (= AGN) Up to many thousand.
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.
WHAT CHANNEL IS THIS? Topic 5. Electromagnetic Radiation Electromagnetic radiation: varying types of energy waves emitted by stars.
Gamma-Ray Bursts Please press “1” to test your transmitter.
Chapter 20: 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.
Observatories: Local & Remote
Radio Loud and Radio Quiet AGN
Chapter 15: Our Galaxy © 2015 Pearson Education, Inc.
Great Ideas in Science: Lecture 8 – Stars & Galaxies
Cherenkov Telescope Array
DIRECT DETECTION OF GRAVITATIONAL WAVES FROM NEUTRON STARS
Stars, Galaxies, and the Universe
Fermi Bubble Z.G.,Xiong.
Extreme Astronomy and Supernovae
For more information, visit
Announcements Final exam is Monday, May 9, at 7:30 am.
Using Telescopes to Observe Electromagnetic Radiation in Space
ASTR 1040 – November 30 Planetarium, December 5
For more information, visit
Chapter 21 Galaxy Evolution
The lifecycles of stars
How Massive Is Supermassive
Neutron Stars and Black Holes
Very High Energy Phenomena in the Universe
Quasars.
High Energy emission from the Galactic Center
What is Astronomy? An overview..
Black Hole Jets Acceleration of jets Collimation of jets
Discussion slide- info from hq. nasa
Stanford Linear Accelerator
Using Technology to See Beyond the Visible
What is Astronomy? An overview..
Black Hole Jets Acceleration of jets Collimation of jets
Quasars and Active Galactic Nuclei
High Energy Astrophysics: problems and expectations
Galaxies With Active Nuclei
Copy week schedule into your agenda and answer the Question of the Day
NOTES: Active Galactic Nuclei (AGN)
Galaxies With Active Nuclei
Science 10 Astronomy Wonder Project, Tamara Markel
What is Astronomy? An overview..
Presentation transcript:

2000 l.y. M87 Astrophysics @ Purdue

Studying the Cosmos through..... Observations Theory Experiment Astro @ Purdue

Astro @ Purdue 9 research-active faculty members covering a wide range of topics Group includes postdoctoral scholars, staff scientists and students Weekly seminar series and journal discussion club

Multi-wavelength Observations Detailed understanding of astrophysical phenomena requires data spanning huge range of energy! Finley, Peterson, Lister, Cui, Lee, Milisavljevic

Gamma-Ray Astronomy (Finley, Lister, Cui) VERITAS: prime gamma ray observatory in Northern Hemisphere (@Mount Hopkins, AZ); hundreds of TeV sources discovered

Astrophysical Jets (Lister) Investigate jets at center of active galaxies using the Very Long Baseline Array (VLBA) with a large sample (400 jets)! Why do some jets produce high energy gamma-rays? 2000 l.y. M87 MOJAVE VLBA Image

The dynamic gamma-ray sky as seen by the Fermi Observatory speed up factor of 1 million: 1 month elapses every 2 seconds

Formation and Evolution of Galaxies (Lee) What are galaxies like in the distant universe? (<20% of current age) How did galaxies grow? Mergers? Collapse of gas around supermassive black holes? Use optical telescopes to study composition, geometry, stellar populations, temperature.

WIYN Observatory 3.5 meter telescope at Kitt Peak, Arizona One degree (gigapixel) camera Multiobject spectrograph Purdue became a partner in 2017

Stellar Explosions (Milisavljevic) Massive stars die in spectacular explosions that can outshine an entire galaxy’s worth of stars Possible to reconstruct the explosion using careful measurements of the remnant Prof. Milisavljevic’s carries out multiwavelength searches for other cosmic explosions Cassiopeia A supernova reconstruction

Theory (Lyutikov, Giannios) Plasma astrophysics Magneto-hydrodynamics Radiative transfer non-thermal high-energy astrophysics pulsar wind nebulae, active galactic nuclei (blackhole physics), gamma-ray bursts, magnetar, jets, tidal disruption events.

Experimental Dark Matter Search (Lang) Most sensitive dark matter experiment to date XENON1T is currently taking data in Gran Sasso, Italy

The Future: Surveys (Peterson) Large Synoptic Survey Telescope (LSST): will survey the entire sky every few days starting in 2020 Peterson’s group has simulated the entire telescope, from emitted star photon to final image LSST will revolutionize our knowledge of asteroids, variable stars, cosmic explosions.

Purdue Department of Physics and Astronomy Thanks! Questions? Purdue Department of Physics and Astronomy