Environs of Bilateral Supernova Remnants with Neutron Stars

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dc.creatorDubner, G.
dc.creatorGiacani, E.
dc.creatorGaensler, B. M.
dc.creatorGoss, W. M.
dc.creatorGreen, A. J.
dc.date2001-12-06
dc.date.accessioned2026-07-07T02:01:43Z
dc.date.available2026-07-07T02:01:43Z
dc.descriptionWe report on Australia Telescope Compact Array (ATCA) HI observations carried out in the direction of bilateral supernova remnants (SNRs) with associated neutron stars: G296.5+10.0 and G320.4--1.2, in a search for the origin of such morphology. From these studies we conclude that in the case of G296.5+10.0, located far from the Galactic plane, the HI distribution has not influenced the present morphology of the SNR. In the case of G320.4--1.2, evolving in a denser medium, the combined action of the central pulsar, PSR B1509-58, with the peculiar distribution of the surrounding medium, has determined the observed characteristics of the SNR.
dc.descriptionto appear in "Neutron Stars in Supernova Remnants" (ASP Conference Proceedings), eds. P.O. Slane and B.M. Gaensler
dc.identifierhttps://arxiv.org/abs/astro-ph/0112155
dc.identifierhttp://arxiv.org/abs/astro-ph/0112155
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3855
dc.subjectAstrophysics
dc.titleEnvirons of Bilateral Supernova Remnants with Neutron Stars
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