HST/NICMOS Imaging Polarimetry of PPNs

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dc.creatorUeta, Toshiya
dc.creatorMurakawa, Koji
dc.creatorMeixner, Margaret
dc.date2003-10-02
dc.date.accessioned2026-07-07T02:09:56Z
dc.date.available2026-07-07T02:09:56Z
dc.descriptionWe present the preliminary results from our HST/NICMOS imaging polarimetry on optically thin PPNs. The data show the dust distribution in an unprecedented detail. The structure of these faint PPNs is revealed via polarization properties of the dust-scattered light without much interference from the bright central star, proving the unique advantages of the technique over simple imaging.
dc.description2 pages, 1 figure; to appear in "Asymmetrical Planetary Nebulae III" editors M. Meixner, J. Kastner, N. Soker, & B. Balick (ASP Conf. Series)
dc.identifierhttps://arxiv.org/abs/astro-ph/0310052
dc.identifierhttp://arxiv.org/abs/astro-ph/0310052
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6621
dc.subjectAstrophysics
dc.titleHST/NICMOS Imaging Polarimetry of PPNs
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