A detailed abundance analysis of the hot post-AGB star ZNG-1 in M10 |
| |
| Authors: | CJ Mooney WRJ Rolleston FP Keenan PL Dufton DL Pollacco HR Magee |
| |
| Institution: | 1Department of Pure and Applied Physics, The Queen's University of Belfast, University Road, Belfast BT7 1NN;2Isaac Newton Group, Apartado de Correos 368, Santa Cruz de La Palma, Tenerife 38780, Canary Islands, Spain;3Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey RH5 6NT |
| |
| Abstract: | We present a model-atmosphere analysis for the bright ( V ～13) star ZNG-1, in the globular cluster M10. From high-resolution ( R ～40 000) optical spectra we confirm ZNG-1 to be a post-asymptotic giant branch (post-AGB) star. The derived atmospheric parameters are T eff=26 500±1000 K and log g =3.6±0.2 dex . A differential abundance analysis reveals a chemical composition typical of hot post-AGB objects, with ZNG-1 being generally metal poor, although helium is approximately solar. The most interesting feature is the large carbon underabundance of more than 1.3 dex. This carbon deficiency, along with an observed nitrogen enhancement relative to other elements, may suggest that ZNG-1 evolved off the AGB before the third dredge-up occurred. Also, iron depletions observed in other similar stars suggest that gas–dust fractionation in the AGB progenitor could be responsible for the observed composition of these objects. However, we need not invoke either scenario since the chemical composition of ZNG-1 is in good agreement with abundances found for a Population II star of the same metallicity. |
| |
| Keywords: | stars: abundances stars: AGB and post-AGB stars: early-type stars: individual: ZNG-1 stars: Population II globular clusters: individual: M10 |
|
|
