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GRB – The Afterglow
GRB – The Afterglow

Radiation pressure and momentum transfer in dielectrics: The
Radiation pressure and momentum transfer in dielectrics: The

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... of the circular velocity curve that should insure accurate streaming motion solutions. We use the uncertainty introduced in the rotation curve by our choice of stellar M/L=0.45±0.15 to define the error in our measured streaming velocities, together with the measured pitch angle uncertainty. Both are ...
The first gravitational-wave source from the isolated evolution of two
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the effect of sublimation temperature dependencies on disk walls
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ExoOrg_NAI

1 - Técnico Lisboa - Universidade de Lisboa
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Sensor Applications of Soft Magnetic Materials Based on

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Dt © 2013 The McGraw-Hill Companies, Inc. All rights reserved
Dt © 2013 The McGraw-Hill Companies, Inc. All rights reserved

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Lecture Notes 16: Magnetic Vector Potential, A; B = Curl A, Magnetostatic Boundary Conditions

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... seminar the practical uses of forces on moving magnets are shown. 1. INTRODUCTION The topic of magnetic braking has dramatically increased in popularity in recent years. Since 1987, numerous articles about magnetic braking were published. These articles describe both experiments dealing with magneti ...
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Potassium abundances in nearby metal-poor stars

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The Diverse Origins of Terrestrial-Planet Systems

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Liquid Rope Coiling

... The origin of liquid-rope coiling effect is based on the un-isotropic nature of the viscous liquid internally, the viscosity plays a significant role to determine whether the phenomenon will be observed or not. The bucking phenomenon is the response of fluid to its impact on substrate and itself is ...
THE GREAT AGN DEBATE `AGN VS STARBURST
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Research paper
Research paper

... of ∼414 pc (Menten et al. 2007; Goddi et al. 2011a) is the densest and most molecule-rich part of the degree-long 2,200 M Integral-Shaped Filament (Johnstone & Bally 1999) in the 50,000 M Orion A cloud (Bally et al. 1987). OMC1 contains the ∼ 1 − 2 × 104 L but visually obscured Becklin-Neugebauer ...
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Accretion disk

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