Radio characteristics of the very young Planetary Nebulae SAO244567

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dc.creatorTrigilio, C.
dc.creatorUmana, G.
dc.creatorCerrigone, L.
dc.date2003-10-10
dc.date.accessioned2026-07-07T02:10:18Z
dc.date.available2026-07-07T02:10:18Z
dc.descriptionThe radio emission from the youngest known Planetary nebula, SAO244567, has been mapped at 20,13, 6, 3.6 and 1.2 cm by using the Australian Telescope Compact Array (ATCA). These observations constitute the first detailed radio study of this very interesting object, as they allow us to obtain, for the first time, the radio morphology of the source and to compute the radio spectrum up to 18752 MHz.
dc.description4 pages, 1 figure; to appear in ``Asymmetric Planetary Nebulae III'', ASP conf. series, in press (2003)
dc.identifierhttps://arxiv.org/abs/astro-ph/0310288
dc.identifierhttp://arxiv.org/abs/astro-ph/0310288
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6696
dc.subjectAstrophysics
dc.titleRadio characteristics of the very young Planetary Nebulae SAO244567
dc.typetext

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