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Date: 2015
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/1235179
Description: The Gum Nebula is 36°-wide shell-like emission nebula at a distance of only ~450 pc. It has been hypothesized to be an old supernova remnant, fossil HⅡ region, wind-blown bubble, or combination of mul ... More
Reviewed: Reviewed
Date: 2015
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/674543
Description: Giant protoplanets evacuate a gap in their host protoplanetary disc, which gas must cross before it can be accreted. A magnetic field is likely carried into the gap, potentially influencing the flow. ... More
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Reviewed: Reviewed
Date: 2015
Language: eng
Resource Type: Thesis PhD
Identifier: http://hdl.handle.net/1959.14/1075051
Description: Thesis by publication.
Full Text: Full Text
Date: 2014
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/307915
Description: The common envelope (CE) interaction describes the swallowing of a nearby companion by a growing, evolving star. CEs that take place during the asymptotic giant branch phase of the primary may lead to ... More
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Reviewed: Reviewed
Date: 2012
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/212670
Description: Magnetic diffusion in accretion flows changes the structure and angular momentum of the accreting material. We present two power-law similarity solutions for flattened accretion flows in the presence ... More
Reviewed: Reviewed
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