HR 62: A New Evolved Chemically Peculiar Late-B Star?

KILIÇOĞLU T., Monier R.

Conference on Radiative Signatures from the Cosmos, Paris, France, 23 - 26 October 2018, vol.519, pp.201-204, (Full Text) identifier

  • Publication Type: Conference Paper / Full Text
  • Volume: 519
  • City: Paris
  • Country: France
  • Page Numbers: pp.201-204
  • Ankara University Affiliated: Yes

Abstract

The spectrum of the evolved B8 III giant HR 62 exhibits weak He-lines and strong Mn and P lines. HR 62 therefore resembles both a HgMn star (CP3) and a He-weak PGa star (CP4).