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Abundance analyses of the new R Coronae Borealis stars ASAS-RCB-8 and ASAS-RCB-10

  • B. P. Hema
  • , Gajendra Pandey
  • , Devika Kamath
  • , N. Kameswara Rao
  • , David Lambert
  • , Vincent M. Woolf

    Research output: Contribution to journal › Article › peer-review

    Abstract

    Abundance analyses of the two newly discovered R Coronae Borealis (RCB) stars ASAS-RCB-8 and ASAS-RCB-10 were conducted using high-resolution optical spectra and model atmospheres. Their chemical compositions place the pair among the majority class of RCBs. ASAS-RCB-10 is one of the most N-poor majority RCBs with an above average O abundance. Relative to ASAS-RCB-10, ASAS-RCB-8 is H poor by 1.6 dex, O-poor by 0.7 dex but N-rich by 0.8 dex suggesting a higher contamination by CNO-cycled material.

    Original languageEnglish
    Article number104202
    Pages (from-to)1-8
    Number of pages8
    JournalPublications of the Astronomical Society of the Pacific
    Volume129
    Issue number980
    DOIs
    Publication statusPublished - 1 Oct 2017

    Keywords

    • stars: abundances
    • stars: chemically peculiar
    • stars: distances

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