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31 October: Supernovae and Neutron Stars
31 October: Supernovae and Neutron Stars

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T3-W10-0501student

... Nuclear fusion no longer takes place, but the star continues to shine with leftover energy. ...
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... An electromagnetic wave (such as a radio wave) propagates outwards from the source (an antenna, perhaps) at the speed of light. What this means in practice is that the source has created oscillating electric and magnetic fields, perpendicular to each other, that travel away from the source. The E an ...
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... “electro-gravity” fields act on the respective individual charges composing the body, with the fields cancelling out exactly at other points. In other words, each “electro-gravity” field acts at the location of the same charge producing it, but the fields together cancel out at other locations. Thus ...
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AWG recommendation on Cosmic Vision

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... stellar remnant. In the remnant, the electrons of atoms are crushed into their nucleus. The star becomes one gigantic atomic nucleus made up only of neutrons – a neutron star. ...
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... On the visualization screen, make sure the picomotor is enabled and that the status is “READY”, and check that output terminal 1 is selected. Then under the “TEMPERATURE” section, click the “Reset Values” button, then click the “Test” button, which will drive the motors continuously for 5 minutes, a ...
The Life Cycles of Stars, Part I
The Life Cycles of Stars, Part I

milano2006_popov - X-Ray
milano2006_popov - X-Ray

... • Our goal is to estimate the number of neutron stars originated from progenitors with enhanced rotation, as such compact objects can be expected to have large magnetic fields, i.e. they can be magnetars. • The fraction of such neutron stars in our calculations is about 8-14 %. • Most of these objec ...
the particle was on Earth`s surface
the particle was on Earth`s surface

... (except at two poles) must rotate in a circle about the Earth’s rotation axis and thus have a centripital acceleration ( requiring a centripital net force ) directed toward the center of the ciecle. ...
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... astronomy and gravitational-waves Astronomy One of the biggest contributions that interferometry has contributed to astronomy is giving an accurate measure of the diameter of stars. Over 100 stellar diameters have been measured, ranging from 0.4 to 5.5 milliarcseconds, sometimes with 1 percent accur ...
Effective field theory methods applied to the 2-body
Effective field theory methods applied to the 2-body

... The existence of gravitational waves (GW) is an unavoidable prediction of General Relativity (GR): any change to a gravitating source must be communicated to distant observers no faster than the speed of light, c, leading to the existence of gravitational radiation, or GWs. The more precise evidence ...
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... The distant galaxy J1148+5251, seen as it was less than 1 billion years after the Big Bang, has a central black hole proportionally larger than those in the nearby universe. Radio observations of this and other distant galaxies suggest that galaxies formed after their black holes. ...
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... The purpose of this paper is to relate the solutions of a conducting shell with uniform charge density to that of hollow earth of uniform mass density. Both problems involve the use of vector superposition within the empty space within each shell. The mathematical form, as a function of densities, p ...
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... • The energy of the star is generated deep down in the core, where the pressure is highest. How does that energy get out? It is transported, and that transport has great bearing on the structure of the star • Early on, you learned there were three energy trnasport mechanisms: conduction, convection ...
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... The former occurs in cool layers, where the gas is partially ionized, while the latter occurs in very hot layers where the energy generation rate is high. Where, or whether, such layers occur in a particular star depends on the mass of the star, as shown in the figure. (c) m/M is the the fraction of ...
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... to perform experiments on nuclei far from stability. RIB facilities will enable us, for the first time, to put our understanding of most of explosive nucleosynthesis and the nature of stellar explosions on a firm experimental basis. The rapid proton capture process (rp-process) Novae and x-ray burst ...
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First observation of gravitational waves

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