'Super massive black hole' diaporamas de présentation

Bijay Kumar Sharma Retired Professor from NITP Currently working in IITP Library

Primary-centric World-View proposes a Fractal Architecture of the Universe- A Post Copernican Conjecture. Bijay Kumar Sharma Retired Professor from NITP Currently working in IITP Library. Post Copernican Conjecture. The Conjecture in colloquial language.

1.17k views • 101 slides

GEARS Workshop Galaxies Sarah Higdon

GEARS Workshop Galaxies Sarah Higdon. Galaxy Evolution. We will test some of the GEARS Galaxy Evolution Unit. There are two goals 1: For everyone to be comfortable with presenting the material in the classrooms.

1.16k views • 98 slides

When ready, please click to begin the game!

Physics. JEOPARDY!. When ready, please click to begin the game!. View Credits. CLICK SCREEN TO CONTINUE >. Gravitation. JEOPARDY!. Who & when. Tides. Black holes. Cosmology. Problems. 100. 100. 100. 100. 100. 200. 200. 200. 200. 200. 300. 300. 300. 300. 300. 400. 400.

568 views • 43 slides

Bellwork

Bellwork. 1. Define AU 2. What do we call the 3 Laws of Planetary Motion?. Chapter 3 Section 4 Planetary Motion Review. Visual Concepts online Ch3Sec4 Planetary Motion worksheet. Create a Chart.

612 views • 40 slides

Supermassive black hole mass J.H. Fan, J.S. Zhang

Third International ASTROD Symposium on Laser Astrodynamics, Space Test of Relativity and Gravitational-Wave Astronomy Beijing, China, July 14 - 16 , 200 6. Supermassive black hole mass J.H. Fan, J.S. Zhang. Center for Astrophysics Guangzhou University. Outline. Introduction Method

545 views • 38 slides

Supermassive black hole mass J.H. Fan, J.S. Zhang

Third International ASTROD Symposium on Laser Astrodynamics, Space Test of Relativity and Gravitational-Wave Astronomy Beijing, China, July 14 - 16 , 200 6. Supermassive black hole mass J.H. Fan, J.S. Zhang. Center for Astrophysics Guangzhou University. Outline. Introduction Method

595 views • 38 slides

Multicolor Microvariability Observations of BL Lac Object: 1ES 1959+650

Multicolor Microvariability Observations of BL Lac Object: 1ES 1959+650. Whitney Wills Advisor: Michael Carini Western Kentucky University. Manufacturer: Group 128 Primary Diameter: 0.6m f-ratio: 11 Design: True Cassegrain Started building process in 1975.

485 views • 33 slides

Super Massive Black Holes!

J ason Liao , A llen Chew May 12th, 2007 C handra A strophysics I nstitute. Super Massive Black Holes!. Outline. Images Our Galaxy images of Sag A Energy Spectrum of Sag A Light Curve of Sag A What is a Super massive Black hole Flux and Luminosity. A Picture of the Milky Way.

278 views • 18 slides

Active Galactic Nuclei

378 views • 16 slides

Search for ~10 17 g Primordial Black Holes with Space-based Gravitational Wave Interferometers

Search for ~10 17 g Primordial Black Holes with Space-based Gravitational Wave Interferometers. Asantha Cooray (Caltech) Based on Seto & Cooray, PRL, astro-ph/0405216 IDM 2004, Edinburgh. Constraints on PBH dark matter. Current constraints on PBH abundance. Lensing, Dymanical, Other

255 views • 15 slides

Active Galactic Nuclei

Active Galactic Nuclei. Nick DiPreta. Nebula. Inside nebula are stellar nurseries Stars begin to form from the gases that are the remnants of past supernovae. Formation of an Average Black Hole. Super Massive Black Hole. Result of a galaxy merger One possible way.

250 views • 13 slides

Active Galactic Nuclei

Active Galactic Nuclei. Nick DiPreta. Nebula. Inside nebula are stellar nurseries Stars begin to form from the gases that are the remnants of past supernovae. Formation of an Average Black Hole. Super Massive Black Hole. Result of a galaxy merger. Super Massive Black Hole.

254 views • 12 slides