Binary hypotheses for bipolar mass loss in transients

<p>We investigate binary hypotheses for the formation of bipolar nebulae using the smoothed particle hydrodynamics code Gadget-2. In the general case, we present a parameter study of mass loss from very simple common envelope models, which seems to show a strongly bipolar trend for sufficientl...

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Main Author: Fitzpatrick, BJR
Other Authors: Podsiadlowski, P
Format: Thesis
Language:English
Published: 2012
Subjects:
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author Fitzpatrick, BJR
author2 Podsiadlowski, P
author_facet Podsiadlowski, P
Fitzpatrick, BJR
author_sort Fitzpatrick, BJR
collection OXFORD
description <p>We investigate binary hypotheses for the formation of bipolar nebulae using the smoothed particle hydrodynamics code Gadget-2. In the general case, we present a parameter study of mass loss from very simple common envelope models, which seems to show a strongly bipolar trend for sufficiently oblate envelopes and low enough spiral-in injection energy. The density profiles of the envelopes produce differing structure within the ejecta.</p> <p>We also investigate 3 specific bipolar mass loss events. In the case of the outer nebula of SN 1987A, we study the effects of fast polar jets interacting with a pre- existing progenitor wind and find that these are consistent with the observed light echoes from the nebula, in particular for the feature known as ’Napoleon’s Hat’. In the case of Cas A, we briefly study the effects of close binarity on supernova ejecta and suggest the influence of a close, compact companion may lead to at least one jet-like disturbance that may be observable in a supernova remnant. Finally, we study whether a fast bipolar wind, similar to that of Eta Car’s present wind, may inflate ejecta similar to that produced in the common envelope models to a shape consistent with that of Eta Car’s Homunculus Nebula.</p>
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spelling oxford-uuid:d3546d77-db00-456b-8bbd-7b3f075ef4a02023-05-04T10:07:02ZBinary hypotheses for bipolar mass loss in transientsThesishttp://purl.org/coar/resource_type/c_db06uuid:d3546d77-db00-456b-8bbd-7b3f075ef4a0Astrophysics (theoretical)EnglishOxford University Research Archive - Valet2012Fitzpatrick, BJRPodsiadlowski, P<p>We investigate binary hypotheses for the formation of bipolar nebulae using the smoothed particle hydrodynamics code Gadget-2. In the general case, we present a parameter study of mass loss from very simple common envelope models, which seems to show a strongly bipolar trend for sufficiently oblate envelopes and low enough spiral-in injection energy. The density profiles of the envelopes produce differing structure within the ejecta.</p> <p>We also investigate 3 specific bipolar mass loss events. In the case of the outer nebula of SN 1987A, we study the effects of fast polar jets interacting with a pre- existing progenitor wind and find that these are consistent with the observed light echoes from the nebula, in particular for the feature known as ’Napoleon’s Hat’. In the case of Cas A, we briefly study the effects of close binarity on supernova ejecta and suggest the influence of a close, compact companion may lead to at least one jet-like disturbance that may be observable in a supernova remnant. Finally, we study whether a fast bipolar wind, similar to that of Eta Car’s present wind, may inflate ejecta similar to that produced in the common envelope models to a shape consistent with that of Eta Car’s Homunculus Nebula.</p>
spellingShingle Astrophysics (theoretical)
Fitzpatrick, BJR
Binary hypotheses for bipolar mass loss in transients
title Binary hypotheses for bipolar mass loss in transients
title_full Binary hypotheses for bipolar mass loss in transients
title_fullStr Binary hypotheses for bipolar mass loss in transients
title_full_unstemmed Binary hypotheses for bipolar mass loss in transients
title_short Binary hypotheses for bipolar mass loss in transients
title_sort binary hypotheses for bipolar mass loss in transients
topic Astrophysics (theoretical)
work_keys_str_mv AT fitzpatrickbjr binaryhypothesesforbipolarmasslossintransients