PLASMA PHYSICS EFFECTS OF HALL CURRENTS ON JEANS’ GRAVITATIONAL INSTABILITY OF ROTATING UNBOUNDED PLASMA AIYUB KHAN1, S.S. TAK1, PRIYADARSHI PATNI2 1

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Question 4. Starting from radiative transfer equation, suppose the source function is a linear a b ,v function of vertical optical depth S ,v (a) Please explain what is limb darkening effect using the surface intensiti

Source URL: www.astro.ncu.edu.tw

• Physical quantities
• Star
• Limb darkening
• Jeans instability
• Free-fall time
• Magnetic field
• Mass
• James Hopwood Jeans
• Physics
• Stellar astronomy
• Astrophysics

M4221: Research Topics in Astrophysics Part II: Star Formation Assignment 1 Dr. Daniel Price April 5, 2011

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• Water waves
• Fluid dynamics
• Physical oceanography
• Jeans instability
• Jeans length
• Wave
• Dispersion relation
• Dispersion
• Instability
• Physics
• Astrophysics
• Wave mechanics

PhD Qualifying Exam (2010) --- 星球天文物理 What is limb darkening? Can the limb darkening be seen if the star were isothermal, that is, the temperature is a constant all over the star? Why? Finally, explain how t

Source URL: www.astro.ncu.edu.tw

• Space
• Star
• Luminosity
• Eddington luminosity
• Sun
• Main sequence
• Limb darkening
• Temperature
• Jeans instability
• Physics
• Astronomy
• Astrophysics

The high-mass slope of the IMF at sub-solar metallicities Simon Glover

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• Initial mass function
• Jeans instability
• Accretion
• Space
• Astrophysics
• Stellar astronomy
• Astronomy