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We present the first three-dimensional simulations of the evolution of a microquasar jet inside the binary-star system. The aim is to study the interaction of these jets with the stellar wind from a m...
It has been suggested that chondrules and calcium-aluminum-rich inclusions (CAIs) were formed at the inner edge of the protoplanetary disk and then entrained in magnetocentrifugal X-winds. We study tr...
The theory of radiatively driven winds successfully explains the key points of the stellar winds of hot massive stars. However, there is an apparent break-down of this paradigm at L/Lsun<5.2: the stel...
In some massive stars, magnetic fields are thought to confine the outflowing radiatively-driven wind. Although theoretical models and MHD simulations are able to illustrate the dynamics of such a magn...
Since the first exoplanet — a planet outside our solar system — was discovered in 1995, more than 460 others have been found. While astronomers have been able to measure the size, orbital characterist...
Supernova Explosions in Winds and Bubbles, with Applications to SN 1987A。
Hadronic gamma-ray production in microquasars with equatorial winds
Accretion of stellar winds in the galactic centre。
Determination of the Mass Loss Rate and the Terminal Velocity of Stellar Winds. I. Genetic Algorithm for Automatic Line Profile Fitting。
Very Large Array Observations of Winds from Massive Stars。
Winds Driven by Super-Star Clusters。
Winds from Low Mass Stars:impact on the ISM。
Protostellar Disks under the Influence of Winds and UV Radiation。
High Resolution X-Ray Observations of Pulsar Winds
High Resolution X-Ray Observations of Pulsar Winds

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