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Dust driven mass loss from carbon stars as function of stellar parameters - II. Effects of grain size on wind properties
AGB and post-AGB – Stars: atmospheres – Stars: carbon – Stars: circumstellar matter – Stars: evolution – Stars: mass loss –2 Hydrodynamics – Radiative transfer
2011/9/30
In this paper we explore grain size effects on wind properties of carbon stars, using a generalized description of radiative cross sections valid for particles of arbitrary sizes. The purpose of the s...
Clustered Star Formation in Magnetic Clouds: Properties of Dense Cores Formed in Outflow-Driven Turbulence
Magnetic Clouds: Properties Dense Cores Formed Outflow-Driven Turbulence
2011/10/11
We investigate the physical properties of dense cores formed in turbulent, magnetized, parsec-scale clumps of molecular clouds, using three-dimensional numerical simulations that include protostellar ...
Radiation-driven winds of hot luminous stars. XVI. Expanding atmospheres of massive and very massive stars and the evolution of dense stellar clusters
Radiation mechanisms: general – Methods: numerical – Radiative transfer – early Universe – Stars: early-type – mass- loss – stellar winds – very massive stars – stellar evolution
2011/9/27
Context: Starbursts, and particularly their high-mass stars, play an essential role in the evolution of galaxies. The winds of massive stars not only significantly influence their surroundings, but th...
The Outer Evolution of Structure in Radiatively Driven Stellar Winds
Radiatively Driven Stellar Winds Outer Evolution of Structure
2009/6/16
The Outer Evolution of Structure in Radiatively Driven Stellar Winds。
The Partition Between Terminal Speed and Mass Loss:Thin, Thick, and Rotating Line-Driven Winds
Terminal Speed Rotating Line-Driven Winds Mass Loss
2009/6/16
The Partition Between Terminal Speed and Mass Loss:Thin, Thick, and Rotating Line-Driven Winds。
Disk formation in Be-stars due to line driven stellar wind and rotation
Be-stars rotation stellar wind
2009/6/10
Disk formation in Be-stars due to line driven stellar wind and rotation。