@inproceedings{30471969deac440daa328682e9d59c2e,
title = "Alfven waves propagation in homogeneous and dusty astrophysical plasmas",
abstract = "Astrophysical plasma coexist with dust particles in many situations. These particles are charged either negatively or positively depending on their surrounding plasma environments. This system of such charged dust, electrons, and ions forms a so-called dusty plasma. We discuss the effects of the dust particles on the propagation and absorption of the Alfven waves in (i) stellar winds and (ii) in star formation regions. In both cases, we have shown the importance of a strong damping of Alfven waves due to the dust and the consequences for wind acceleration and the changes in the Jeans length related to the star formation process. (c) 2005 COSPAR. Published by Elsevier Ltd. All rights reserved.",
keywords = "Alfven waves, magnetized dusty plasmas, wave propagation, LOW-FREQUENCY WAVES, WOLF-RAYET STARS, STELLAR WINDS, MASS-LOSS, MOLECULAR CLOUDS, CIRCUMSTELLAR ENVELOPE, PHYSICAL CONDITIONS, RADIATION PRESSURE, SIZE DISTRIBUTION, MAGNETIC-FIELDS",
author = "{de Juli}, MC and D Falceta-Goncalves and V Jatenco-Pereira",
year = "2005",
doi = "10.1016/j.asr.2005.03.143",
language = "English",
series = "ADVANCES IN SPACE RESEARCH",
publisher = "PERGAMON-ELSEVIER SCIENCE LTD",
pages = "925--935",
editor = "V Jatenco-Pereira and ACL Chian and JF ValdesGalicia and MA Shea",
booktitle = "Fundamentals of Space Environment Science",
note = "1st Latin-American Advanced School on Space Environment ; Conference date: 22-03-2004 Through 27-03-2004",
}