Stellar Rotation and the Formation of Asymmetric Nebulae

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dc.creatorDwarkadas, Vikram V.
dc.date2004-01-07
dc.date.accessioned2026-07-07T02:11:48Z
dc.date.available2026-07-07T02:11:48Z
dc.descriptionWe illustrate how rotation of the central star can give rise to latitudinal variations in the wind properties from the star. Interaction of these winds with the surrounding medium can produce asymmetrical planetary nebulae.
dc.description4 pages; to appear in Asymmetric Planetary Nebulae III, eds. M. Meixner, J. Kastner, N.Soker and B. Balick (ASP Conf. Ser.)
dc.identifierhttps://arxiv.org/abs/astro-ph/0401066
dc.identifierhttp://arxiv.org/abs/astro-ph/0401066
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7228
dc.subjectAstrophysics
dc.titleStellar Rotation and the Formation of Asymmetric Nebulae
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