The Circumstellar Matter Around OH44.8-2.3

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dc.creatorBobrowsky, M.
dc.creatorGreeley, B. W.
dc.creatorUeta, T.
dc.creatorMeixner, M. M.
dc.date2000-01-07
dc.date.accessioned2026-07-07T01:51:36Z
dc.date.available2026-07-07T01:51:36Z
dc.descriptionI-band images of the OH maser source OH44.8-2.3 are presented. Having a well-determined distance, this object is shown to be very young and physically small, with an asymmetric compact bipolar nebula already present. In the morphological terminology of Meixner et al. (2000) and Ueta et al. (2000), this object would be classified as a DUPLEX nebula because of its high optical depth and pole-to-equator density contrast.
dc.descriptionTo appear in ``Asymmetrical Planetary Nebulae II: from Origins to Microstructures,'' ASP Conference Series, Vol. 199, 2000; J.H. Kastner, N. Soker, & S.A. Rappaport, eds
dc.identifierhttps://arxiv.org/abs/astro-ph/0001115
dc.identifierhttp://arxiv.org/abs/astro-ph/0001115
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/351
dc.subjectAstrophysics
dc.titleThe Circumstellar Matter Around OH44.8-2.3
dc.typetext

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