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UVA - PHYS - 605
Carousels and Roller Coasters 1Carousels and Roller Coasters 2Question: Carousels and Roller Coasters When the wine glass was directly above my head, was there a force pushing up on the wine glass that kept the glass against the tray?Carousels
UVA - PHYS - 605
Falling Balls 1Falling Balls 2Question: Falling BallsSuppose that I throw a ball upward into the air. After the ball leaves my hand, is there any force pushing the ball upward?Falling Balls 3Falling Balls 4Observations About Falling Balls
UVA - PHYS - 605
Seesaws 1Seesaws 2Question: Seesaws You and a child half your height lean out over the edge of a pool at the same angle. If you both let go simultaneously, who will tip over faster and hit the water first?Seesaws 3Seesaws 4Observations Abo
UVA - PHYS - 605
Water Distribution 1Water Distribution 2Question: Water Distribution Water enters your home plumbing at ground level. Where will you get the strongest spray from a shower? In the ground floor shower In the basement shower In the second floor
UVA - PHYS - 605
Wheels 1Wheels 2Question: Wheels You are in a tremendous hurry and you want your car to accelerate as quickly as possible when the light turns green. Tire damage is not an issue. Will you accelerate faster if you "burn rubber" (skid your wheels)
UVA - PHYS - 631
Lecture 5 Friday July 13 Chapter 8Continuation of Conservation of Energy Two Sample Problems Spread sheet problem for you Hand out last years exam Misconception problems quitExternal Work (No Friction)BallW (eg. I could lift the ball) Ball-Ear
UVA - PHYS - 606
Physics Chat Room March 19 2008You are free to type text in the text line anytime. If you want to speak, click on the hand and I will give you the floor. Do this now just to say hello Agenda None of the questions in the chat room are graded. Start
UVA - PHYS - 606
Welcome to the Phys 606 Chat Room 8-9 PM Feb 20You are free to type text in the text line anytime. If you want to speak, click on the hand and I will give you the floor. Do this now just to say hello Then I will review some topics Focus on elementar
UVA - PHYS - 606
University of Virginia Department of PhysicsPhysics 606: How Things Work IILecture #20 Slides: Audio AmplifiersRecording Tape Sound current sent through ring-shaped electromagnet Split in ring develops north and south poles Nearby tape regio
UVA - PHYS - 606
University of Virginia Department of PhysicsPhysics 606: How Things Work IILecture #30 Slides: Fluorescent Lights IIAtomic Structure Electrons travel as waves Electron in an orbital doesn't emit light Electron emits light when changing orbit
UVA - PHYS - 606
University of Virginia Department of PhysicsPhysics 606: How Things Work IILecture #38 Slides: Nuclear Weapons IIStructure of Nucleus Nucleus contains two kinds of nucleons Protons are positively charged Neutrons are neutralNuclear Stabili
UVA - PHYS - 606
University of Virginia Department of PhysicsPhysics 606: How Things Work IILecture #22 Slides: ComputersQuestion: ComputersToday, the fastest PCs run at roughly 1.5 GHz. Someday, computers may run at 1,000,000 GHz. Compared to present computer
UVA - PHYS - 606
Question Previewerhttp:/www.webassign.net/v4cgiral5q@virginia/questions/previe.Case 2-3 - Bumper Cars (354474)Test / Preview Code Show New Randomization Open in Editor Print Show: All, None Key Solution Help/Hints MarkBumper cars are a popular
UVA - PHYS - 606
University of Virginia Department of PhysicsPhysics 606: How Things Work IILecture #36 Slides: Windows and Glass II and PlasticsTempered Glass Tempering glass Heat glass to softening point Cool outside of glass quickly Outside stiffens whil
UVA - PHYS - 606
University of Virginia Department of PhysicsPhysics 606: How Things Work IILecture #7 Slides: WheelsQuestion: WheelsYou are in a tremendous hurry and you want your car to accelerate as quickly as possible when the light turns green. Tire damag
UVA - PHYS - 606
University of Virginia Department of PhysicsPhysics 606: How Things Work IILecture #16 Slides: Power DistributionPower Power is energy per unit of time Power is measured in joules/second or watts Batteries are power sources Loads are power
UVA - PHYS - 606
University of Virginia Department of PhysicsPhysics 606: How Things Work IILecture #24 Slides: Radios IITank Circuit Inductor & Capacitor share energy Charge flows back and forth through inductor Energy shifts back and forth between the two
UVA - PHYS - 606
University of Virginia Department of PhysicsPhysics 606: How Things Work IILecture #4 Slides: Force and WorkPhysics Concept Net Force The sum of all forces on an object. Determines object's acceleration.Newton's Third LawFor every force t
UVA - PHYS - 606
University of Virginia Department of PhysicsPhysics 606: How Things Work IILecture #14 Slides: Magnetically Levitated Trains II and FlashlightsElectromagnetic Induction Changing magnetic field electric field Electric field in conductor cu
UVA - PHYS - 606
University of Virginia Department of PhysicsPhysics 606: How Things Work IILecture #12 Slides: Xerographic Copiers IIMetals The Fermi level has empty levels just above it Like patrons in a partly fill theatre, electrons can move in response t
UVA - PHYS - 606
University of Virginia Department of PhysicsPhysics 606: How Things Work IILecture #34 Slides: Knives and SteelQuestion: Knives and SteelIf you take a steel paper clip and bend it repeatedly, will it become stiffer or less stiff with each new
UVA - PHYS - 606
University of Virginia Department of PhysicsPhysics 606: How Things Work IILecture #1 Slides: Introduction to course and SkatingQuestion: SkatingA rotary lawn mower spins its sharp blade rapidly over the lawn and cuts the tops of the grasses o
UVA - PHYS - 606
University of Virginia Department of PhysicsPhysics 606: How Things Work IILecture #26 Slides: MicrowavesQuestion:If you put a CD in a microwave oven, it willMicrowave Ovens1. do nothing. 2. burn up the microwave oven. 3. burn up the CD.O
UVA - PHYS - 606
Welcome to the Phys 606 Chat Room 8-9 PM Apr 16 You are free to type text in the text line anytime. If you want to speak, Click on the hand and I will give you the floor. We all should do this just to say hello Then I will review selected topics.
UVA - PHYS - 606
University of Virginia Department of PhysicsPhysics 606: How Things Work IILecture #5 Slides: SeesawsWork Lifting Ball Going straight up: Force is large Distance is smallForces on a RampSupport Net Forcedistancework =force Weight
UVA - CS - 101
Applications of Scientific Computing9. Scientific ComputingScience and engineering challenges.! !Commercial applications.! !!!!!!!!!!Fluid dynamics. Seismic surveys. Plasma dynamics. Ocean circulation. Electronics design.
UVA - CS - 101
Overview4.1 - 4.2 Analysis of AlgorithmsAnalysis of algorithms. Framework for comparing algorithms and predicting performance. Scientific method. Observe some feature of the universe. Hypothesize a model that is consistent with observation. Predi
UVA - CS - 686
Dependable ComputingDependable Computing CS686John C. Knight Department of Computer Science University of Virginia knight@cs.virginia.edu 434.982.2216 John C. Knight, 2009 - All rights reserved.Beginning of Course MemoReadit is on the Web site
UVA - SBB - 801
!" " ) ( )# !$% & % " ( " , % . ( %'" * +""," / (,)( -/ " ) 1 ( 2 * % " ( ( %" " " ( 3 ) ( ( ( (" *( ( 0 % + 4 " ( "*) #5 6$ " " ( % 4( % )/0 ) ( ( ( ( # ! 9 &: " " * ) " / " " / 7 " / 7 ) 89% " ") ' ) (* " $% %
UVA - AE - 554
Components of Galaxies Gas The Importance of Gas Fuel for star formation (H2) Tracer of galaxy kinematics/mass (HI) Tracer of dynamical history of interaction between galaxies (HI)Much of this material has been / will be covered in your ISM
UVA - AST - 554
Components of Galaxies Gas The Importance of Gas Fuel for star formation (H2) Tracer of galaxy kinematics/mass (HI) Tracer of dynamical history of interaction between galaxies (HI)Much of this material has been / will be covered in your ISM
UVA - AE - 554
AST 554 - Homework #1Due February 24, 2009 Note: This homework covers some of the topics in the preliminary lectures up through "Components of Galaxies: Gas". The problems are intended to be relatively straight-forward. Please remember to define al
UVA - AST - 554
AST 554 - Homework #1Due February 24, 2009 Note: This homework covers some of the topics in the preliminary lectures up through "Components of Galaxies: Gas". The problems are intended to be relatively straight-forward. Please remember to define al
UVA - AE - 554
Components of Galaxies: Dark MatterDark Matter: Any Form of matter whose existence is inferred solely through its gravitational effects. -B&T, pg 590 Nature of Major Component of Universe Galaxy Formation Fate of the UniverseEvidence for Dark M
UVA - AST - 554
Components of Galaxies: Dark MatterDark Matter: Any Form of matter whose existence is inferred solely through its gravitational effects. -B&T, pg 590 Nature of Major Component of Universe Galaxy Formation Fate of the UniverseEvidence for Dark M
UVA - AE - 554
The Astrophysical Journal, 686:948965, 2008 October 20# 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A.ATHE RESOLVED PROPERTIES OF EXTRAGALACTIC GIANT MOLECULAR CLOUDSAlberto D. Bolatto,1 Adam K. Leroy,2 Erik Ros
UVA - AST - 554
The Astrophysical Journal, 686:948965, 2008 October 20# 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A.ATHE RESOLVED PROPERTIES OF EXTRAGALACTIC GIANT MOLECULAR CLOUDSAlberto D. Bolatto,1 Adam K. Leroy,2 Erik Ros
UVA - AE - 554
The Astrophysical Journal, 629:6171, 2005 August 10# 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A.THE RELATIONSHIP BETWEEN LUMINOSITY AND BROAD-LINE REGION SIZE IN ACTIVE GALACTIC NUCLEIShai Kaspi,1, 2 Dan Maoz,1
UVA - AST - 554
The Astrophysical Journal, 629:6171, 2005 August 10# 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A.THE RELATIONSHIP BETWEEN LUMINOSITY AND BROAD-LINE REGION SIZE IN ACTIVE GALACTIC NUCLEIShai Kaspi,1, 2 Dan Maoz,1
UVA - AE - 554
THE ASTROPHYSICAL JOURNAL, 507 : 615654, 1998 November 10( 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.ROTATING NUCLEAR RINGS AND EXTREME STARBURSTS IN ULTRALUMINOUS GALAXIES D. DOWNESInstitut de Radio Astronomi
UVA - AST - 554
THE ASTROPHYSICAL JOURNAL, 507 : 615654, 1998 November 10( 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.ROTATING NUCLEAR RINGS AND EXTREME STARBURSTS IN ULTRALUMINOUS GALAXIES D. DOWNESInstitut de Radio Astronomi
UVA - AE - 554
The Astronomical Journal, 124:788810, 2002 August# 2002. The American Astronomical Society. All rights reserved. Printed in U.S.A.MOLECULAR GAS IN ELLIPTICAL GALAXIES: DISTRIBUTION AND KINEMATICS L. M. YoungPhysics Department, New Mexico Institut
UVA - AST - 554
The Astronomical Journal, 124:788810, 2002 August# 2002. The American Astronomical Society. All rights reserved. Printed in U.S.A.MOLECULAR GAS IN ELLIPTICAL GALAXIES: DISTRIBUTION AND KINEMATICS L. M. YoungPhysics Department, New Mexico Institut
UVA - AST - 554
1997MNRAS.289.766H1997MNRAS.289.766H1997MNRAS.289.766H1997MNRAS.289.766H1997MNRAS.289.766H1997MNRAS.289.766H1997MNRAS.289.766H1997MNRAS.289.766H1997MNRAS.289.766H1997MNRAS.289.766H1997MNRAS.289.766H1997MNRAS.289.766H1997MNRAS.
UVA - AE - 554
1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.34
UVA - AST - 554
1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.343.1D1989ApJ.34
UVA - AST - 554
1995ARA&A.33.581K1995ARA&A.33.581K1995ARA&A.33.581K1995ARA&A.33.581K1995ARA&A.33.581K1995ARA&A.33.581K1995ARA&A.33.581K1995ARA&A.33.581K1995ARA&A.33.581K1995ARA&A.33.581K1995ARA&A.33.581K1995ARA&A.33.581K1995ARA&A.33.581K199
UVA - AE - 554
1976ApJ.203.297S1976ApJ.203.297S1976ApJ.203.297S1976ApJ.203.297S1976ApJ.203.297S1976ApJ.203.297S1976ApJ.203.297S1976ApJ.203.297S1976ApJ.203.297S1976ApJ.203.297S
UVA - AST - 554
1976ApJ.203.297S1976ApJ.203.297S1976ApJ.203.297S1976ApJ.203.297S1976ApJ.203.297S1976ApJ.203.297S1976ApJ.203.297S1976ApJ.203.297S1976ApJ.203.297S1976ApJ.203.297S
UVA - AE - 554
THE ASTROPHYSICAL JOURNAL, 478 : 144161, 1997 March 20( 1997. The American Astronomical Society. All rights reserved. Printed in U.S.A.THE MOLECULAR INTERSTELLAR MEDIUM IN ULTRALUMINOUS INFRARED GALAXIES P. M. SOLOMONAstronomy Program, State Univ
UVA - AST - 554
THE ASTROPHYSICAL JOURNAL, 478 : 144161, 1997 March 20( 1997. The American Astronomical Society. All rights reserved. Printed in U.S.A.THE MOLECULAR INTERSTELLAR MEDIUM IN ULTRALUMINOUS INFRARED GALAXIES P. M. SOLOMONAstronomy Program, State Univ
UVA - AE - 554
1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S
UVA - AST - 554
1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S1983ApJ.265.148S
UVA - AE - 554
Population Synthesis Models: ColorColor DiagramModelsDataComponents of Galaxies: Dust Is efficient at absorbing UV and optical light, and thus affects the interpretation of the emission at these wavelengths (e.g., stellar population synt
UVA - AST - 554
Population Synthesis Models: ColorColor DiagramModelsDataComponents of Galaxies: Dust Is efficient at absorbing UV and optical light, and thus affects the interpretation of the emission at these wavelengths (e.g., stellar population synt
UVA - AE - 554
Components of Galaxies Stars What Properties of Stars are Important for Understanding Galaxies?(Ref: B&M 5.1, S&G 2.2) Temperature Determines the range over which the radiation is emitted Chemical Composition metallicities Lifetimes Determin
UVA - AST - 554
Components of Galaxies Stars What Properties of Stars are Important for Understanding Galaxies?(Ref: B&M 5.1, S&G 2.2) Temperature Determines the range over which the radiation is emitted Chemical Composition metallicities Lifetimes Determin
UVA - AST - 554
1987ApJ.320.238S1987ApJ.320.238S1987ApJ.320.238S1987ApJ.320.238S1987ApJ.320.238S1987ApJ.320.238S1987ApJ.320.238S1987ApJ.320.238S1987ApJ.320.238S1987ApJ.320.238S1987ApJ.320.238S1987ApJ.320.238S1987ApJ.320.238S1987ApJ.320.238S
UVA - AST - 554
1984ApJ.285.89D1984ApJ.285.89D1984ApJ.285.89D1984ApJ.285.89D1984ApJ.285.89D1984ApJ.285.89D1984ApJ.285.89D1984ApJ.285.89D1984ApJ.285.89D1984ApJ.285.89D1984ApJ.285.89D1984ApJ.285.89D1984ApJ.285.89D1984ApJ.285.89D1984ApJ.285.
UVA - AST - 554
1983QJRAS.24.267H1983QJRAS.24.267H1983QJRAS.24.267H1983QJRAS.24.267H1983QJRAS.24.267H1983QJRAS.24.267H1983QJRAS.24.267H1983QJRAS.24.267H1983QJRAS.24.267H1983QJRAS.24.267H1983QJRAS.24.267H1983QJRAS.24.267H1983QJRAS.24.267H198