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M sun
M sun

ch07-4 - Physics-YISS
ch07-4 - Physics-YISS

... Elastic collision -- One in which the total kinetic energy of the system after the collision is equal to the total kinetic energy before the collision. Inelastic collision -- One in which the total kinetic energy of the system after the collision is not equal to the total kinetic energy before the c ...
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... • The positive is taken if currents I1 and I2 flow such that the magnetic fields of the two circuits strengthen each other. See table 8.3 in textbook with formulas for inductance of common elements like coaxial cable, two-wire line, etc. ...
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... the star formation community. It is now viewed as a common, though still poorly understood, phenomenon in low-mass star formation. The FU Orionis objects (FUors) are long-studied examples of this phenomenon. FUors are believed to undergo accretion outbursts during which the accretion rate rapidly in ...
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... In the semiclassical Bohr model of the hydrogen atom, the electron moves in a circular orbit of radius 0.53x10-10 m with speed = 2.2x106 m/s. According to this model, what is the magnetic field at the center of a hydrogen atom? (Problem 32.73) ...
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PHYS3380_111815_bw - The University of Texas at Dallas

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... Polars are a type of CV that has a strong magnetic field around 100 million times earths magnetic field. The plasma is not allowed to form an accretion disc because it follows the magnetic field lines. The stream takes a more direct path toward the white dwarf. The high speeds of the impacting parti ...
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Accretion disk

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