L
Lister Staveley-Smith
Researcher at University of Western Australia
Publications - 615
Citations - 40651
Lister Staveley-Smith is an academic researcher from University of Western Australia. The author has contributed to research in topics: Galaxy & Large Magellanic Cloud. The author has an hindex of 95, co-authored 599 publications receiving 36924 citations. Previous affiliations of Lister Staveley-Smith include University of West Alabama & Australian Astronomical Observatory.
Papers
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Journal ArticleDOI
Fractal Structure in the Interstellar Medium of the Small Magellanic Cloud
TL;DR: In this article, the authors used the spatial power spectrum for a statistical study of HI in the SMC in order to probe the intrinsic topology of the ISM and found that a remarkable power-law fit to the SP spectrum was found, supporting an alternative ISM model having a fractal nature resulting from interstellar turbulence.
Journal ArticleDOI
An H I mosaic of the Small Magellanic Cloud.
Lister Staveley-Smith,Robert J. Sault,David McConnell,M. J. Kesteven,Despina Hatzidimitriou,Kenneth C. Freeman,Michael A. Dopita +6 more
Book ChapterDOI
Studying galaxy formation in loose galaxy groups
Daniel J. Pisano,Daniel J. Pisano,David G. Barnes,Brad K. Gibson,Lister Staveley-Smith,Kenneth C. Freeman,Virginia A. Kilborn +6 more
TL;DR: In this paper, the authors present the results of a HI survey of six loose groups of galaxies analogous to the Local Group, and discuss the possible role of HVCs in solving the ''missing satellite'' problem.
Journal ArticleDOI
The Arecibo L-band Feed Array Zone of Avoidance (ALFAZOA) Shallow Survey
Monica Sanchez-Barrantes,Monica Sanchez-Barrantes,P. A. Henning,T. McIntyre,Emmanuel Momjian,Robert F. Minchin,Jessica L. Rosenberg,Stephen E. Schneider,Lister Staveley-Smith,W. van Driel,M. Ramatsoku,Z. Butcher,E. Vaez +12 more
Proceedings ArticleDOI
Connecting the Baryons: Multiwavelength Data for SKA HI Surveys
Martin Meyer,Aaron S. G. Robotham,Danail Obreschkow,Simon P. Driver,Lister Staveley-Smith,Martin Zwaan +5 more
TL;DR: As they evolve, galaxies experience a host of environmental and feedback influences, manyof which can radically impact their gas content as mentioned in this paper, and the result of these processes can significantly alter the baryonic states in which materialis finally observed (stellar populations, dust, chemistry) and its morphology (galaxy type,bulge/disk ratio, bars, warps, radial pro�le).