Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2157
Title: R Coronae Borealis stars at minimum light - UW Cen
Authors: Kameswara Rao, N
Reddy, B. E
Lambert, D. L
Keywords: stars: individual: UW Cen;stars: variables: other
Issue Date: Dec-2004
Publisher: Blackwell Publishing
Citation: Monthly Notices of the Royal Astronomical Society, Vol. 355, No. 3, pp. 855 – 861
Abstract: Two high-resolution optical spectra of the R Coronae Borealis (R CrB) star UW Cen in decline are discussed. A spectrum from mid-1992 when the star had faded by 3 mag shows just a few differences with the spectrum at maximum light. The ubiquitous sharp emission lines seen in R CrB at a similar drop below maximum light are absent. In contrast, a spectrum from mid-2002 when the star was 5 mag below maximum light shows an array of sharp emission lines and a collection of broad emission lines. Comparisons are made with spectra of R CrB obtained during the deep 1995–1996 minimum. The many common features are discussed in terms of a torus-jet geometry.
URI: http://hdl.handle.net/2248/2157
???metadata.dc.relation.uri???: http://www.blackwell-synergy.com/doi/abs/10.1111/j.1365-2966.2004.08363.x
http://arxiv.org/abs/astro-ph/0409211
Appears in Collections:IIAP Publications

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