RRI Digital Repository >
04. Astronomy and Astrophysics >
Research Papers (A&A) >
Please use this identifier to cite or link to this item:
|Title: ||HI Density Distribution Driven by Supernovae:A Simulation Study|
|Authors: ||Hodge, Jacqueline A.|
|Issue Date: ||Jul-2007 |
|Publisher: ||Astronomical Society of the Pacific|
|Citation: ||ASP Conference Series, Vol. 365, 2007, p158-161|
|Abstract: ||We model the complex distribution of atomic hydrogen (HI) in the interstellar medium (ISM) assuming that it is driven entirely by supernovae (SN). We describe the simulations and present our results in the form of spatial distributions and the associated power spectra. In both of two approaches explored here, we find remarkable correspondence with the observed statistical description of well-studied components of the ISM, wherein the spatial spectra have been found to show significant deviations from the Kolmogorov spectrum.|
|Description: ||Restricted Access.
SINS - Small Ionized and Neutral Structures in the Diffuse Interstellar Medium. ASP Conference Series, Vol. 365, Proceedings of the conference held 21-24 May, 2006 at the National Radio Astronomy Observatory in Socorro, New Mexico, USA. Edited by M. Haverkorn and W. M. Goss.|
|Alternative Location: ||http://adsabs.harvard.edu/cgi-bin/bib_query?2007ASPC..365..158H|
|Copyright: ||2007 Astronomical Society of the Pacific|
|Appears in Collections:||Research Papers (A&A)|
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.