Observational Ponderings on Disk-Halo Interfaces

Details Observational Ponderings on Disk-Halo Interfaces Observational Ponderings on Disk-Halo Interfaces

Jun 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..331..147g&link_type=abstract

Extra-Planar Gas, ASP Conference Proceedings, Vol. 331. Edited by Robert Braun. Proceedings of the meeting held at Dwingeloo,

Astronomy and Astrophysics

Astronomy

2

Scientific paper

In considering the structures of disk-halo boundaries, it is important to include the range of possible halo structures. These can be roughly divided between quasi-static halos that are in near equilibrium states and halos that evolve in response to gas or power inflows from embedded disks or the wider surroundings. Superwinds in starburst galaxies are extreme examples of evolving halos, and we consider the nature of such systems from the perspective of new studies of the archetypal starburst galaxy, M82.

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