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Date: 2014
Resource Type: Thesis PhD
Identifier: http://hdl.handle.net/1959.14/337736
Description: Bibliography: pages 387-442.
Full Text: Full Text
Authors: Hyde, Elaina, A
Date: 2014
Language: eng
Resource Type: Thesis professional doctorate
Identifier: http://hdl.handle.net/1959.14/1068805
Description: "A thesis submitted to Macquarie University for the degree of Doctor Philosophy, Department of Physics and Astronomy"
Full Text: Full Text
Date: 2012
Language: eng
Resource Type: conference paper
Identifier: http://hdl.handle.net/1959.14/207142
Description: This paper presents an overview of recent progress at the Sydney University Stellar Interferometer (SUSI). Development of the third-generation PAVO beam combiner has continued. The MUSCA beam combiner ... More
Full Text: Full Text
Reviewed: Reviewed
Date: 2011
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/140073
Description: We continue our study of weakly ionized protostellar accretion discs that are threaded by a large-scale magnetic field and power a centrifugally driven wind. It has been argued that there is already e ... More
Reviewed: Reviewed
Date: 2010
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/1148615
Description: A concise summary of the recent international workshop held in honour of the career of Agǹs Acker is presented together with a brief exposition of her productive career in the study of Planetary Nebul ... More
Date: 2009
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/1142467
Description: PILOT (the Pathfinder for an International Large Optical Telescope) is a proposed 2.5-m optical/ infrared telescope to be located at Dome C on the Antarctic plateau. Conditions at Dome C are known to ... More
Reviewed: Reviewed
Date: 2008
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/1169394
Description: A ring of dense molecular gas extending 2-7 pc orbits the supermassive black hole Sgr A at the center of our Galaxy. Using the Green Bank Telescope, we detected water maser lines and both narrow (0.35 ... More
Reviewed: Reviewed
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