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Classification of Ionized Photoevaporation Flows

Published online by Cambridge University Press:  13 May 2016

W.J. Henney
W.J. Henney*
Affiliation:
Instituto de Astronomía, UNAM Campus Morelia, Michoacán, México

Abstract

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From proplyds to champagne flows, spanning 4 orders of magnitude in size and density, photoevaporation flows are ubiquitous in H II regions. Such flows are also found in planetary nebulae, in the form of cometary knots, although in this case the flows are often “advection-dominated”, unlike the “recombination-dominated” flows that predominate in H II regions.

Information

Type
Star Formation Regions and Outflow Processes in our Galaxy
Information
Symposium - International Astronomical Union , Volume 205: Galaxies and their Constituents at the Highest Angular Resolutions , 2001 , pp. 272 - 273
Copyright
Copyright © Astronomical Society of the Pacific 2001 

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