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Spectral variations of DY Cen
Authors:Sunetra Giridhar  N Kameswara Rao  David L Lambert
Institution:(1) Indian Institute of Astrophysics, 560034 Bangalore, India;(2) Department of Astronomy, University of Texas, 78712 Austin, TX, USA
Abstract:Two high resolution spectra of the hot RCrB star DY Cen in the red region are compared. The photospheric absorption lines show a radial velocity variation of 12 kms-1 between 1989 July and 1992 May. Emission components to some CII lines present in 1989 are almost entirely absent in 1992. Nebular forbidden lines of OI], NII] and SII] appear unchanged from 1989 to 1992
Keywords:Hot RCrB stars  radial velocity  photospheric and nebular lines
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