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      Permanent link:
      https://www.ias.ac.in/article/fulltext/joaa/017/01-02/0023-0040

    • Keywords

       

      Hot RCrB stars; radial velocity; photospheric and nebular lines

    • 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

    • Author Affiliations

       

      Sunetra Giridhar1 N. Kameswara Rao1 David L. Lambert2

      1. Indian Institute of Astrophysics, Bangalore - 560034, India
      2. Department of Astronomy, University of Texas, Austin, TX - 78712, USA

    • Dates

       
      Published
      June 1996
      Manuscript received
      7 February 1996
      Accepted
      29 March 1996

  • Journal of Astrophysics and Astronomy | News

    • Continuous Article Publication

      Posted on January 27, 2016

      Since January 2016, the Journal of Astrophysics and Astronomy has moved to Continuous Article Publishing (CAP) mode. This means that each accepted article is being published immediately online with DOI and article citation ID with starting page number 1. Articles are also visible in Web of Science immediately. All these have helped shorten the publication time and have improved the visibility of the articles.

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