Two New Close Binary Central Stars of Planetary Nebulae from a Critically Selected Southern Hemisphere Sample

Simple item page
dc.creatorHillwig, Todd C.
dc.date2003-10-01
dc.date.accessioned2026-07-07T02:09:55Z
dc.date.available2026-07-07T02:09:55Z
dc.descriptionI present the results of time-resolved photometry of a selection of central stars of planetary nebulae. The study reveals periodic variability in two of the eight central stars observed, those of NGC 6026 and NGC 6337. The variability matches that expected from a binary system in which a hot primary irradiates a cooler secondary star.
dc.descriptionTo appear in "Asymmetrical Planetary Nebulae III", eds. M. Meixner, J. H. Kastner, and N. Soker, ASP Conf. Series; 4 pages, 4 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0310043
dc.identifierhttp://arxiv.org/abs/astro-ph/0310043
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6615
dc.subjectAstrophysics
dc.titleTwo New Close Binary Central Stars of Planetary Nebulae from a Critically Selected Southern Hemisphere Sample
dc.typetext

Files

Collections

arXiv