Spectral analysis of the hybrid PG 1159-type central stars of the planetary nebulae Abell 43 and NGC 7094

Stellar post asymptotic giant branch (post-AGB) evolution can be completely altered by a final thermal pulse (FTP) which may occur when the star is still leaving the AGB (AFTP), at the departure from the AGB at still constant luminosity (late TP, LTP) or after the entry to the white-dwarf cooling se...

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Autores principales: Löbling, L., Rauch, Thomas, Miller Bertolami, Marcelo Miguel, Todt, Helge, Friederich, Felix, Ziegler, M., Werner, Klaus, Kruk, Jeffrey W.
Formato: Articulo
Lenguaje:Inglés
Publicado: 2019
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/125467
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id I19-R120-10915-125467
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
Astronomía
stars: abundances
stars: AGB and post-AGB
stars: atmospheres
stars: evolution
stars: individual: WD 1751 + 106
stars: individual: WD 2134 + 125
spellingShingle Ciencias Astronómicas
Astronomía
stars: abundances
stars: AGB and post-AGB
stars: atmospheres
stars: evolution
stars: individual: WD 1751 + 106
stars: individual: WD 2134 + 125
Löbling, L.
Rauch, Thomas
Miller Bertolami, Marcelo Miguel
Todt, Helge
Friederich, Felix
Ziegler, M.
Werner, Klaus
Kruk, Jeffrey W.
Spectral analysis of the hybrid PG 1159-type central stars of the planetary nebulae Abell 43 and NGC 7094
topic_facet Ciencias Astronómicas
Astronomía
stars: abundances
stars: AGB and post-AGB
stars: atmospheres
stars: evolution
stars: individual: WD 1751 + 106
stars: individual: WD 2134 + 125
description Stellar post asymptotic giant branch (post-AGB) evolution can be completely altered by a final thermal pulse (FTP) which may occur when the star is still leaving the AGB (AFTP), at the departure from the AGB at still constant luminosity (late TP, LTP) or after the entry to the white-dwarf cooling sequence (very late TP, VLTP). Then convection mixes the He-rich material with the H-rich envelope. According to stellar evolution models the result is a star with a surface composition of H≈20 per cent by mass (AFTP), ≈ 1 per cent (LTP), or (almost) no H (VLTP). Since FTP stars exhibit intershell material at their surface, spectral analyses establish constraints for AGB nucleosynthesis and stellar evolution. We performed a spectral analysis of the so-called hybrid PG 1159-type central stars (CS) of the planetary nebulae Abell 43 and NGC 7094 by means of non-local thermodynamical equilibrium models. We confirm the previously determined effective temperatures of T<sub>eff</sub>=115000±5000K and determine surface gravities of log(g/(cms<sup>−2</sup>))=5.6±0.1 for both. From a comparison with AFTP evolutionary tracks, we derive stellar masses of 0.57<sup>+0.07</sup><sub>−0.04</sub> M⊙ and determine the abundances of H, He, and metals up to Xe. Both CS are likely AFTP stars with a surface H mass fraction of 0.25 ± 0.03 and 0.15 ± 0.03, respectively, and an Fe deficiency indicating subsolar initial metallicities. The light metals show typical PG 1159-type abundances and the elemental composition is in good agreement with predictions from AFTP evolutionary models. However, the expansion ages do not agree with evolution time-scales expected from the AFTP scenario and alternatives should be explored.
format Articulo
Articulo
author Löbling, L.
Rauch, Thomas
Miller Bertolami, Marcelo Miguel
Todt, Helge
Friederich, Felix
Ziegler, M.
Werner, Klaus
Kruk, Jeffrey W.
author_facet Löbling, L.
Rauch, Thomas
Miller Bertolami, Marcelo Miguel
Todt, Helge
Friederich, Felix
Ziegler, M.
Werner, Klaus
Kruk, Jeffrey W.
author_sort Löbling, L.
title Spectral analysis of the hybrid PG 1159-type central stars of the planetary nebulae Abell 43 and NGC 7094
title_short Spectral analysis of the hybrid PG 1159-type central stars of the planetary nebulae Abell 43 and NGC 7094
title_full Spectral analysis of the hybrid PG 1159-type central stars of the planetary nebulae Abell 43 and NGC 7094
title_fullStr Spectral analysis of the hybrid PG 1159-type central stars of the planetary nebulae Abell 43 and NGC 7094
title_full_unstemmed Spectral analysis of the hybrid PG 1159-type central stars of the planetary nebulae Abell 43 and NGC 7094
title_sort spectral analysis of the hybrid pg 1159-type central stars of the planetary nebulae abell 43 and ngc 7094
publishDate 2019
url http://sedici.unlp.edu.ar/handle/10915/125467
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