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... Models of the chemical evolution of our Galaxy are extended to include radial migration of stars and flow of gas through the disc. The models track the production of both iron and alpha elements. A model is chosen that provides an excellent fit to the metallicity distribution of stars in the Geneva- ...
PHY101 Quiz#3 - People Server at UNCW
PHY101 Quiz#3 - People Server at UNCW

... 2. Melissa's favorite exercise equipment at the gym consists of various springs. In one exercise, she pulls a handle grip attached to the free end of a spring to 0.80 m from its unstrained position. The other end of the spring (spring constant = 45 N/m) is held in place by the equipment frame. What ...
Galactic Center problem sheet
Galactic Center problem sheet

... where rs = 2GM• /c2 is the Schwarzschild radius and it is the radius of the sphere around the mass M• from which the escape velocity is equal to the speed of light. This null hypersurface is characterized by the infinite redshift for the observer at infinity and is commonly referred to as the event ...
Chapter 15: Oscillations 15-23 THINK The maximum force that can
Chapter 15: Oscillations 15-23 THINK The maximum force that can

WinFinal
WinFinal

... 8. (a) Find the charge distribution q(r) inside a sphere which carries a charge density proportional to the distance from the origin,  = c r, for some constant c. [Hint: A spherical volume element is d= r2 sin dr d d where (0<<) and (0<).] (b) Sketch q(r) and (r). (c) Find the electri ...
1. In a rectangular area shown in the figure uniform magnetic field of
1. In a rectangular area shown in the figure uniform magnetic field of

... perpendicular to the plane of the paper is present. A proton is arriving at the boundary of the magnetic field with constant velocity of v = 107 m/s perpendicular to the magnetic field. The mass and the charge of the proton are me = 1.67 × 10−27 kg and Qp = 1.6 × 10−19 C, respectively. d = 0.3 m. a. ...
2-2 Approach
2-2 Approach

22. The Milky Way Galaxy
22. The Milky Way Galaxy

Document
Document

AST101 Lecture 20 The Ecology of the Galaxy
AST101 Lecture 20 The Ecology of the Galaxy

Short theoretical questions – solutions
Short theoretical questions – solutions

... Let α be the angle between the vectors p and Δp, and β between the radius vector of the satellite and the vector Δp. By thinking about the direction of the additional impulse Δp, consider if it is possible to change the orbit to each of the cases given below. If it is possible mark YES on the answer ...
Great Migrations & other natural history tales
Great Migrations & other natural history tales

Rigid_Body_Dynamics1..
Rigid_Body_Dynamics1..

PPT
PPT

Astrophysics 14 - Black Holes
Astrophysics 14 - Black Holes

Optical studies of an ultraluminous X-ray source: NGC1313 X-2 Jifeng Liu
Optical studies of an ultraluminous X-ray source: NGC1313 X-2 Jifeng Liu

Solutions - faculty.ucmerced.edu
Solutions - faculty.ucmerced.edu

The Milky Way as a Galaxy, Galaxy Classification
The Milky Way as a Galaxy, Galaxy Classification

final-S06
final-S06

Work and Power 13.1
Work and Power 13.1

Characterizing Extrasolar Planetary Systems
Characterizing Extrasolar Planetary Systems

1.2 Characterize gas and ice giant exoplanets to constrain
1.2 Characterize gas and ice giant exoplanets to constrain

Protoplanetary disks, jets, and the birth of the stars
Protoplanetary disks, jets, and the birth of the stars

Wednesday, June 25, 2008
Wednesday, June 25, 2008

Chapter 8 Rotational Dynamics continued
Chapter 8 Rotational Dynamics continued

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Accretion disk

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