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.
Deshpande, A.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.
ISBN: 978-1-583812-33-4
Alternative Location:
Copyright: 2007 Astronomical Society of the Pacific
Appears in Collections:Research Papers (A&A)

Files in This Item:
File Description SizeFormat 
2007 ASP Conf. Series V365 p158.pdf
  Restricted Access
Restricted Access274.13 kBAdobe PDFView/Open Request a copy

Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.