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A common feature of the X-ray bubbles observed in Chandra images of some "cooling flow" clusters is that they appear to be surrounded by bright, cool shells. Temperature maps of a few nearby luminous ...
The first stars and quasars are known sources of hard ionizing radiation in the first billion years of the Universe. We examine the joint effects of X-rays and hard UV radiation from such first-light ...
The ISM, powered by SNe, is turbulent and permeated by a magnetic field (with a mean and a turbulent component). It constitutes a frothy medium that is mostly out of equilibrium and is ram pressure do...
The cosmological remnants of a first-order phase transition generally depend on the perturbations that the walls of expanding bubbles originate in the plasma. Several of the formation mechanisms occur...
Wind-Blown Bubbles and HII Regions around Massive Stars。
Supernova Explosions in Winds and Bubbles, with Applications to SN 1987A。
Wind-Blown Bubbles around Massive Stars. The effects of stellar wind and photo-ionization on the circumstellar Medium。
Photon Bubbles in Young Massive Stars。
Planetary Nebulae, Bubbles and Superbubbles:What Can We Learn From Their Kinematics?
An Inside-Out View of Bubbles     Bubbles  Inside-Out View       2009/6/15
An Inside-Out View of Bubbles
Neutral Gas Bubbles Surrounding Southern Optical Ring Nebulae:Anon (WR 23) and RCW 52。
Stellar Wind Bubbles:H-Deficient Stars and X-Ray Spectra。
Multipolar Bubbles, Point-Symmetry and Jets in Dying Stars。
Winds, Bubbles, ...but Magnetized: solutions for High Speed Post-AGB Winds and their Extreme Collimation。
Bubbles, bow-shocks, and bullets over broad-lines:three ionized outflows resolved with hst。

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