Holes and Shells in Galaxies: Observations versus Theoretical Concepts

Details Holes and Shells in Galaxies: Observations versus Theoretical Concepts Holes and Shells in Galaxies: Observations versus Theoretical Concepts

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998mcdg.proc...67p&link_type=abstract

The Magellanic Clouds and Other Dwarf Galaxies, Proceedings of the Bonn/Bochum-Graduiertenkolleg Workshop, held at the Physikzen

Other

Neutral Hydrogen, Shells

Scientific paper

Shells and holes discovered in the distribution of H I in the Milky Way and nearby galaxies within 10 Mpc are reviewed. To interpret the data, the hydrodynamical equations in 1D and 2D, and equations describing the expansion of infinitesimally thin shell in 2D and 3D, have been used. The abundance and distribution of holes and shells in the Milky Way, Magellanic Clouds, and other nearby galaxies are discussed and conditions for shell fragmentation and propagating star formation are evaluated.

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