2-D Radiation Transfer Model of Non-Spherically Symmetric Dust Shell in P roto-Planetary Nebulae

Simple item page
dc.creatorSu, K. Y. L.
dc.creatorVolk, K.
dc.creatorKwok, S.
dc.date2000-01-05
dc.date.accessioned2026-07-07T01:51:33Z
dc.date.available2026-07-07T01:51:33Z
dc.descriptionWe have fitted the HST images and the spectral energy distributions (SEDs) of three proto-planetary nebulae (PPN) with a 2-D radiation transfer model. The geometric and mass loss properties of these PPN are also derived.
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/0001069
dc.identifierhttp://arxiv.org/abs/astro-ph/0001069
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/334
dc.subjectAstrophysics
dc.title2-D Radiation Transfer Model of Non-Spherically Symmetric Dust Shell in P roto-Planetary Nebulae
dc.typetext

Files

Collections

arXiv