Molecules as Tracers of PN Structure

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dc.creatorHuggins, P. J.
dc.date2000-01-29
dc.date.accessioned2026-07-07T01:51:57Z
dc.date.available2026-07-07T01:51:57Z
dc.descriptionMolecular gas plays an important role in the structure of planetary nebulae: it is a major component of the equatorial tori of bipolar nebulae, it forms the cores of globules and related mircostructures, and is the likely origin of multiple arcs. It is also a key component during the early stages of formation where interactions with outflows or jets provide an important shaping mechanism.
dc.descriptionTo appear in ``Asymmetrical Planetary Nebulae II: from Origins to Microstructures'', ASP Conference Series, Vol. 199, 2000; J.H. Kastner, N. Soker, and S.A. Rappaport, eds
dc.identifierhttps://arxiv.org/abs/astro-ph/0001518
dc.identifierhttp://arxiv.org/abs/astro-ph/0001518
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/468
dc.subjectAstrophysics
dc.titleMolecules as Tracers of PN Structure
dc.typetext

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