A&A 438, 23-29 (2005)
DOI: 10.1051/0004-6361:20052972
Solitary waves in self-gravitating molecular clouds
T. Cattaert1 and F. Verheest1, 21 Sterrenkundig Observatorium, Universiteit Gent, Krijgslaan 281, 9000 Gent, Belgium
e-mail: Frank.Verheest@UGent.be
2 School of Physics (Howard College Campus), University of KwaZulu-Natal, Durban 4041, South Africa
(Received 2 March 2005 / Accepted 8 April 2005)
Abstract
Molecular clouds are self-gravitating fluids that support different waves
and contain highly nonlinear clumps and filaments, for which explanations
have been sought in terms of solitons.
The present paper explores the possibility that several (neutral) species
with different thermal speeds coexist, as in a molecular cloud consisting
of gas and dust, or of a mixture of normal matter and dark matter.
It is shown that this model can support soliton formation, both with humps
or dips in the self-gravitational potential.
The existence domain has been given in terms of the hot species Mach
number and fractional mass density, in a gas-dynamic description which
emphasizes the constraints coming from the sonic and neutral points, and
from the limits due to infinite compression or total rarefaction.
One species is compressed while the other is rarefied, allowing the system
to reach a mass neutral point outside equilibrium.
In this way, solitons are possible without invoking interaction with a
weakly ionized cloud component or involving envelope solitons that are not
really stationary structures.
Key words: gravitation -- hydrodynamics -- ISM: clouds -- waves
© ESO 2005
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