Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100330136> ?p ?o ?g. }
- W3100330136 endingPage "15" @default.
- W3100330136 startingPage "15" @default.
- W3100330136 abstract "Post-asymptotic giant branch (post-AGB) stars are known to be chemically diverse. In this paper we present the first observational evidence of a star that has failed the third dredge-up (TDU). J005252.87-722842.9 is a A-type ($T_{rm eff}$ = 8250 $pm$ 250K) luminous (8200 $pm$ 700 $rm L_{odot}$), metal-poor ($textrm{[Fe/H]}$ = $- 1.18 pm$ 0.10), low-mass (M$_{rm initial}$ $approx$ 1.5 $-$ 2.0 $rm M_{odot}$) post-AGB star in the Small Magellanic Cloud. Through a systematic abundance study, using high-resolution optical spectra from UVES, we found that this likely post-AGB object shows an intriguing photospheric composition with no confirmed carbon-enhancement (upper limit of [C/Fe] $<$ 0.50) nor enrichment of $s$-process elements. We derived an oxygen abundance of [O/Fe] = 0.29 $pm$ 0.1. For Fe and O, we took into account the effects of non-local thermodynamic equilibrium (NLTE). We could not derive an upper limit for the nitrogen abundance as there are no useful nitrogen lines within our spectral coverage. The chemical pattern displayed by this object has not been observed in single or binary post-AGBs. Based on its derived stellar parameters and inferred evolutionary state, single star nucleosynthesis models predict that this star should have undergone TDU episodes while on the AGB and be carbon-enriched. However, our observations are in contrast with these predictions. We identify two possible Galactic analogues which are likely to be post-AGB stars, but the lack of accurate distances (hence luminosities) to these objects does not allow us to confirm their post-AGB status. If they have low luminosities then they are likely to be dusty post-RGB stars. The discovery of J005252.87-722842.9 reveals a new stellar evolutionary channel whereby a star evolves without any third dredge-up episodes." @default.
- W3100330136 created "2020-11-23" @default.
- W3100330136 creator A5000235602 @default.
- W3100330136 creator A5008721221 @default.
- W3100330136 creator A5024091569 @default.
- W3100330136 creator A5055412533 @default.
- W3100330136 creator A5066643989 @default.
- W3100330136 creator A5088116706 @default.
- W3100330136 date "2017-02-06" @default.
- W3100330136 modified "2023-09-25" @default.
- W3100330136 title "Discovery of a Metal-poor, Luminous Post-AGB Star that Failed the Third Dredge-up" @default.
- W3100330136 cites W133143164 @default.
- W3100330136 cites W1790922966 @default.
- W3100330136 cites W1877064744 @default.
- W3100330136 cites W1963836638 @default.
- W3100330136 cites W1970520663 @default.
- W3100330136 cites W1971972731 @default.
- W3100330136 cites W1972474208 @default.
- W3100330136 cites W1973932881 @default.
- W3100330136 cites W1978738088 @default.
- W3100330136 cites W1990850583 @default.
- W3100330136 cites W1998934211 @default.
- W3100330136 cites W2003135449 @default.
- W3100330136 cites W2004500012 @default.
- W3100330136 cites W2009399375 @default.
- W3100330136 cites W2010494516 @default.
- W3100330136 cites W2019472482 @default.
- W3100330136 cites W2021714225 @default.
- W3100330136 cites W2034477498 @default.
- W3100330136 cites W2035363165 @default.
- W3100330136 cites W2035816776 @default.
- W3100330136 cites W2046033763 @default.
- W3100330136 cites W2047510114 @default.
- W3100330136 cites W2049474854 @default.
- W3100330136 cites W2066607243 @default.
- W3100330136 cites W2066946006 @default.
- W3100330136 cites W2075971915 @default.
- W3100330136 cites W2077456416 @default.
- W3100330136 cites W2086209426 @default.
- W3100330136 cites W2088153665 @default.
- W3100330136 cites W2091754576 @default.
- W3100330136 cites W2092108498 @default.
- W3100330136 cites W2094180700 @default.
- W3100330136 cites W2095644639 @default.
- W3100330136 cites W2109010002 @default.
- W3100330136 cites W2114584474 @default.
- W3100330136 cites W2114908771 @default.
- W3100330136 cites W2115358257 @default.
- W3100330136 cites W2129527325 @default.
- W3100330136 cites W2129528413 @default.
- W3100330136 cites W2129566255 @default.
- W3100330136 cites W2132358681 @default.
- W3100330136 cites W2132963711 @default.
- W3100330136 cites W2133385779 @default.
- W3100330136 cites W2151136987 @default.
- W3100330136 cites W2158710097 @default.
- W3100330136 cites W2160068792 @default.
- W3100330136 cites W2160944361 @default.
- W3100330136 cites W2167635287 @default.
- W3100330136 cites W2225046757 @default.
- W3100330136 cites W2248595088 @default.
- W3100330136 cites W2263412961 @default.
- W3100330136 cites W2473546813 @default.
- W3100330136 cites W2480004221 @default.
- W3100330136 cites W2517710328 @default.
- W3100330136 cites W2522000147 @default.
- W3100330136 cites W2899497983 @default.
- W3100330136 cites W3098804378 @default.
- W3100330136 cites W3099032735 @default.
- W3100330136 cites W3099833547 @default.
- W3100330136 cites W3099844113 @default.
- W3100330136 cites W3100016480 @default.
- W3100330136 cites W3100029030 @default.
- W3100330136 cites W3100215491 @default.
- W3100330136 cites W3100656076 @default.
- W3100330136 cites W3101364261 @default.
- W3100330136 cites W3101664312 @default.
- W3100330136 cites W3101671574 @default.
- W3100330136 cites W3101834416 @default.
- W3100330136 cites W3102683676 @default.
- W3100330136 cites W3102949007 @default.
- W3100330136 cites W3103945413 @default.
- W3100330136 cites W3104013109 @default.
- W3100330136 cites W3104204533 @default.
- W3100330136 cites W3106147843 @default.
- W3100330136 cites W3106164066 @default.
- W3100330136 cites W3106265688 @default.
- W3100330136 cites W3123451623 @default.
- W3100330136 cites W4290042936 @default.
- W3100330136 cites W4292399985 @default.
- W3100330136 cites W4295032385 @default.
- W3100330136 doi "https://doi.org/10.3847/1538-4357/836/1/15" @default.
- W3100330136 hasPublicationYear "2017" @default.
- W3100330136 type Work @default.
- W3100330136 sameAs 3100330136 @default.
- W3100330136 citedByCount "11" @default.
- W3100330136 countsByYear W31003301362018 @default.
- W3100330136 countsByYear W31003301362019 @default.