HST NICMOS Observation of Proto-Planetary Nebulae

Simple item page
dc.creatorSu, K. Y. L.
dc.creatorKwok, S.
dc.creatorHrivnak, B. J.
dc.creatorSahai, R.
dc.date2000-01-06
dc.date.accessioned2026-07-07T01:51:35Z
dc.date.available2026-07-07T01:51:35Z
dc.descriptionWe report NICMOS wide-band and polarimetric observations of four proto-planetary nebulae. Molecular hydrogen emission is detected near the ends of the bipolar lobes of IRAS 17150-3224, which is evidence for the interaction of a fast, collimated outflow with the remnant of the asymptotic giant branch wind.
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/0001097
dc.identifierhttp://arxiv.org/abs/astro-ph/0001097
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/341
dc.subjectAstrophysics
dc.titleHST NICMOS Observation of Proto-Planetary Nebulae
dc.typetext

Files

Collections

arXiv