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In order to understand which process (e.g. galactic winds, cold accretion) is responsible for the cool (T~10^4 K) halo gas around galaxies, we embarked on a program to study the star-formation propert...
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...
Rapidly rotating stars show short-period oscillations in magnetic activity and polar appearance of starspots. The aim of this paper is to study large-scale shallow water waves in the tachoclines of ra...
In recent years, a phenomenological solar wind heating model based on a turbulent energy cascade prescribed by the Kolmogorov theory has produced reasonably good agreement with observations on proton ...
Whether the phenomenology governing MHD turbulence is Kolmogorov or Iroshnikov-Kraichnan (IK) remains an open question, theoretically as well as observationally. The ion heating profile observed in th...
The Emission from Photoionized Stellar Wind Bow Shocks。
The Interaction of a Jet-Like Pulse with a Wind from a Stellar Companion。
Hydrodynamical Interaction between an Accretion Flow and a Stellar Wind
Wind-Blown Bubbles around Massive Stars. The effects of stellar wind and photo-ionization on the circumstellar Medium。
[WC] Stellar wind turbulent outflows feeding the ism。
Disk formation in Be-stars due to line driven stellar wind and rotation。
New VLA Observations of WR 6 (= HR 50896): A Search for an Anisotropic Wind

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