This site uses cookies. By continuing to use this site you agree to our use of cookies. To find out more, see our Privacy and Cookies policy. Close this notification
The American Astronomical Society, find out more

Click here to close this overlay, or press the "Escape" key on your keyboard.

The American Astronomical Society (AAS), established in 1899 and based in Washington, DC, is the major organization of professional astronomers in North America. Its membership of about 7,000 individuals also includes physicists, mathematicians, geologists, engineers, and others whose research and educational interests lie within the broad spectrum of subjects comprising contemporary astronomy. The mission of the AAS is to enhance and share humanity's scientific understanding of the universe.

https://aas.org/

The Institute of Physics, find out more

Click here to close this overlay, or press the "Escape" key on your keyboard.

The Institute of Physics (IOP) is a leading scientific society promoting physics and bringing physicists together for the benefit of all. It has a worldwide membership of around 50 000 comprising physicists from all sectors, as well as those with an interest in physics. It works to advance physics research, application and education; and engages with policy makers and the public to develop awareness and understanding of physics. Its publishing company, IOP Publishing, is a world leader in professional scientific communications.

https://www.iop.org

Extreme Scattering Events and Galactic Dark Matter

and

Published 1998 April 21 © 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Mark Walker and Mark Wardle 1998 ApJ 498 L125

1538-4357/498/2/L125

Abstract

"Extreme scattering events" (ESEs) are attributed to radio wave refraction by a cloud of free electrons crossing the line of sight. We present a new model in which these electrons form the photoionized "skin" of an underlying cool, self-gravitating cloud in the Galactic halo. In this way, we avoid the severe overpressure problem that afflicts other models. The UV flux in the Galactic halo naturally generates electron densities of the right order. We demonstrate, for the first time, a good reproduction of the prototypical ESE in the quasar 0954+658. The neutral clouds are a few astronomical units in radius and have masses ≲10-3 M. The observed rate of ESEs implies that a large fraction of the mass of the Galaxy is in this form.

Export citation and abstract BibTeX RIS

Please wait… references are loading.
10.1086/311332