Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Swinburne
U. Colorado
Univ. Central Lancashire, UK
University of Central Lancashire
Swinburne University
Centre for Astrophysics & Supercomputing, Swinburne University
Swinburne University & ULancashire
MSSSO
Centre for Astrophysics, University of Central Lancashire
The HIPASS team
U. of Colorado
UofC
CASA
Centre for Astrophysics, University of Central Lancashire, Preston, PR1 2HE, UK; School of Physics, University of Sydney, NSW, 2006, Australia
Centre for Astrophysics and Supercomputing, Swinburne University of Technology, PO Box 218, Hawthorn, VIC 3122, Australia
MSSO
Centre for Astrophysics, University of Central Lancashire, Preston, PR1 2HE, UK
Swinburne University of Technology, Mail Number 31, P.O. Box 218, Hawthorn, Victoria 3122, Australia.
Center for Astrophysics and Space Astronomy, Department of Astrophysical and Planetary Sciences, University of Colorado, Boulder, CO 80309
CU / CASA
Swinburne University of Technology
Univ. of Colorado
UC Lancashire
UCLan
Central Lancashire
Swinburne Univ.
UCLan, UK
MSSSO,Oxford,UBC
Center for Astrophysics & Supercomputing, Swinburne University
JHI
University of Oxford
UCLan / St. Mary's
University of Colorado
Centre for Astrophysics and Supercomputing, Swinburne University, P.O. Box 218, Hawthorn, VIC 3122, Australia of Colorado and University of Wisconsin
Jeremiah Horrocks Institute, University of Central Lancashire, Preston, PR1 2HE, UK
British Columbia Univ., Vancouver.
Centre for Astrophysics and Supercomputing, Swinburne University, P.O. Box 218, Hawthorn, VIC 3122, Australia
British Columbia, University, Vancouver, Canada
British Columbia Univ., Vancouver, Canada
A Catalog of H I-Selected Galaxies from the South Celestial Cap Region of Sky
A Catalogue of Field Horizontal Branch Stars Aligned with High Velocity Clouds
A Cepheid Distance to the Fornax Cluster
A Cepheid distance to the Fornax cluster and the local expansion rate of the Universe
A Comparison of Galaxy Group Luminosity Functions from Semi-Analytic Models
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