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Instruments for Gravitational Wave Astronomy on Ground and in Space
Instruments for Gravitational Wave Astronomy on Ground and in Space

... objects are mainly compact systems involving neutron stars or black holes ending by an inspiral phase of variable time duration. Systems involving objects of stellar class (up to a few tens of solar masses) on compact orbits emit gravitational waves (GW) roughly in the acoustic band (from a few Hz t ...
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Wide-field surveys and astronomical discovery space

Metric Expansion of Space Described by Gravity Based on
Metric Expansion of Space Described by Gravity Based on

... We do not know the starting position, velocity or direction of our part of space relative to the singularity. However, observations display that space that we can observe expands at an increasing speed [8]-[10]. The present theoretical model may explain this metric expansion of space. The model indi ...
Gamma Ray Bursts: The biggest bang since the big one!
Gamma Ray Bursts: The biggest bang since the big one!

... Gravity: warped spacetime • More gravity, deeper hole in spacetime, higher velocity to escape more mass or smaller size • Black hole – escape velocity is faster than light so can’t get out! • No change in curvature at Earths orbit – black holes don’t suck ...
SolarEnergy_Kit#1 - Institute for School Partnership
SolarEnergy_Kit#1 - Institute for School Partnership

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5 December 2012 Atmospheric Phenomena Professor Carolin

... mountaintops are excellent places for watching the skies, whether or not they’re clear! In doing so I have stumbled upon many of the atmospheric phenomena that I’m going to discuss in today’s lecture. Some are relatively predictable and some occur very commonly; others are far rarer, and you are ver ...
HS-SCI-CP -- Chapter 14- Refraction
HS-SCI-CP -- Chapter 14- Refraction

... Refraction can be explained in terms of the wave model of light In the previous chapter on light and refraction, you learned how to use wave fronts and light rays to approximate light waves. This analogy can be extended to light passing from one medium into another. In Figure 3, the wave fronts are ...
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Studying Gravitational Perturbations of Planet Venus by timing of

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Astronomical Facts `n Stuff

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100 Years of Einstein`s Photoelectric Effect

... spores floating in water, moving randomly all the time. Albert Einstein made the first satisfactory theoretical treatment of the Brownian motion in 1905. Einstein's theory [8] enabled significant statistical predictions about the motion of particles that are randomly distributed in a fluid. These pr ...
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Q -1 name some phenomena associated with light. ans – 1) image

... - this is because, the sunlight constitutes parallel rays of light. this rays are concentrated at a sharp bright spot formed on the paper. the concentration of the sunlight at a point generates heat which causes the paper to burn. Q -79 what is principal focus of a convex lens? ans – the point on t ...
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superbubbles vs super-galactic winds

... all the energetics from the starburst. Being massive, although smaller in numbers, they also reinsert into the ISM, through their winds and SN explosions, almost 40% of the starburst original mass. And thus from a starburst with an initial mass of 106 M one has to expect a total of almost 4 ×105 M ...
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General Astronomy Dark Matter

... particles, they must be moving very fast. This sort of dark matter is called ‘Hot Dark Matter” or HDM, because hot particles move fast. • When the universe was young, HDM would move around so fast that it would tend to smooth out small scale density fluctuations. – Any small region which is denser t ...
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Black Hole`` Systems.`

... accretion disk. The magnetic propeller also creates radial outflows of atomic nuclei (shown in indigo blue) and relativistic jets of electrons (shown in red) along the rotation axis. A bright blue-white ring forms where the MECO's rotating magnetic field sweeps the inner edge of the accretion disk, ...
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... Angle, the light will move along the surface of the medium • If the angle of incidence is greater than the Critical Angle, the light ray will reflect ...
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Optics Packet

... intersection. Thus, the normal line for each of these incident rays passes through C.) Measure the angle of incidence and use the law of reflection to construct five reflected rays at the appropriate angle of reflection. For each reflected ray, construct extensions of the rays backwards behind the m ...
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Formation of spiral and elliptical galaxies in a CDM cosmogony

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Layers of the Sun Test 1 study guide. Intoduction to Stars

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... • Find that some are related Large Mass  Large Brightness • Determine model of stellar formation and life cycle ...
Phys 102 * Lecture 2
Phys 102 * Lecture 2

... The man is standing in front of a short flat mirror that is placed too high, so he can only see down to his knees ...
Phys 102 – Lecture 17
Phys 102 – Lecture 17

... The man is standing in front of a short flat mirror that is placed  too high, so he can only see down to his knees ...
Lab 15 How Many Galaxies Are There in the
Lab 15 How Many Galaxies Are There in the

... This is a pretty amazingly large number. Consider that each galaxy has billions of stars, and think just for minute about how many total stars there are in the Universe! It makes you feel pretty small.... but, on the other hand, think how cool it is that humans have evolved to the point where they c ...
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glossary of optical terms

Deep $ I $-band imaging of $ z=\ mathsf {5.99} $ quasar
Deep $ I $-band imaging of $ z=\ mathsf {5.99} $ quasar

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Gravitational lens

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