3D Simulations of the Local Bubble

dc.creatorBreitschwerdt, Dieter
dc.creatorde Avillez, Miguel A.
dc.date2004-02-18
dc.date2004-02-22
dc.date.accessioned2026-07-25T12:12:17Z
dc.descriptionWe have performed high resolution 3D simulations of the Local Bubble (with 1.25 pc finest resolution) in a realistic background ISM, jointly with the dynamical evolution of the neighbouring Loop I superbubble. We can reproduce (i) the size of the bubbles (in contrast to similarity solutions), (ii) the interaction shell with Loop I, discovered with ROSAT, (iii) predict the merging of the two bubbles in about 3 Myr, when the interaction shell starts to fragment, and, (iv) the generation of blobs like the Local Cloud as a consequence of a dynamical instability.
dc.description2 pages, 2 simulation images in jpeg format, to appear in the proceedings of ``From Observations to Self-Consistent Modelling of the ISM in Galaxies'', M.A. de Avillez and D. Breitschwerdt (eds.), Kluwer
dc.identifierhttps://arxiv.org/abs/astro-ph/0402446
dc.identifierhttp://arxiv.org/abs/astro-ph/0402446
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/8276
dc.subjectAstrophysics
dc.title3D Simulations of the Local Bubble
dc.typetext

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