FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W4308248434> ?p ?o ?g. }

• W4308248434 endingPage "A17" @default.
• W4308248434 startingPage "A17" @default.
• W4308248434 abstract "Aims. Stars with strong enhancements of r-process elements are rare and tend to be metal-poor, generally with [Fe/H] < −2 dex, and located in the halo. In this work, we aim to investigate a candidate r-process enriched bulge star with a relatively high metallicity of [Fe/H] ~ − 0.65 dex and to compare it with a previously published r-rich candidate star in the bulge. Methods. We reconsidered the abundance analysis of a high-resolution optical spectrum of the red-giant star 2MASS J18082459-2548444 and determined its europium (Eu) and molybdenum (Mo) abundance, using stellar parameters from five different previous studies. Applying 2MASS photometry, Gaia astrometry, and kinematics, we estimated the distance, orbits, and population membership of 2MASS J18082459-2548444 and a previously reported r-enriched star 2MASS J18174532-3353235. Results. We find that 2MASS J18082459-2548444 is a relatively metal-rich, enriched r-process star that is enhanced in Eu and Mo, but not substantially enhanced in s -process elements. There is a high probability that it has a Galactic bulge membership, based on its distance and orbit. We find that both stars show r-process enhancement with elevated [Eu/Fe]-values, even though 2MASS J18174532-3353235 is 1 dex lower in metallicity. Additionally, we find that the plausible origins of 2MASS J18174532-3353235 to be either that of the halo or the thick disc. Conclusions. We conclude that 2MASS J18082459-2548444 represents the first example of a confirmed r -process enhanced star confined to the inner bulge. We assume it is possibly a relic from a period of enrichment associated with the formation of the bar." @default.
• W4308248434 created "2022-11-09" @default.
• W4308248434 creator A5004226024 @default.
• W4308248434 creator A5025090986 @default.
• W4308248434 creator A5028301941 @default.
• W4308248434 creator A5035719690 @default.
• W4308248434 creator A5039552721 @default.
• W4308248434 creator A5058242812 @default.
• W4308248434 creator A5058696335 @default.
• W4308248434 date "2022-12-23" @default.
• W4308248434 modified "2023-10-17" @default.
• W4308248434 title "First <i>r</i>-process enhanced star confirmed as a member of the Galactic bulge" @default.
• W4308248434 cites W147232447 @default.
• W4308248434 cites W1903699604 @default.
• W4308248434 cites W1942800319 @default.
• W4308248434 cites W1967602533 @default.
• W4308248434 cites W1973022378 @default.
• W4308248434 cites W1975213576 @default.
• W4308248434 cites W1990845972 @default.
• W4308248434 cites W1991240238 @default.
• W4308248434 cites W1992749708 @default.
• W4308248434 cites W2003236861 @default.
• W4308248434 cites W2011301426 @default.
• W4308248434 cites W2016846163 @default.
• W4308248434 cites W2037024160 @default.
• W4308248434 cites W2039873083 @default.
• W4308248434 cites W2043911339 @default.
• W4308248434 cites W2046613319 @default.
• W4308248434 cites W2050677931 @default.
• W4308248434 cites W2055516151 @default.
• W4308248434 cites W2058804003 @default.
• W4308248434 cites W2060135539 @default.
• W4308248434 cites W2062513796 @default.
• W4308248434 cites W2079823603 @default.
• W4308248434 cites W2089630383 @default.
• W4308248434 cites W2091238769 @default.
• W4308248434 cites W2098592245 @default.
• W4308248434 cites W2103165993 @default.
• W4308248434 cites W2117914263 @default.
• W4308248434 cites W2121480729 @default.
• W4308248434 cites W2131795696 @default.
• W4308248434 cites W2135625048 @default.
• W4308248434 cites W2140137154 @default.
• W4308248434 cites W2155066650 @default.
• W4308248434 cites W2164159860 @default.
• W4308248434 cites W2166132860 @default.
• W4308248434 cites W2166193059 @default.
• W4308248434 cites W2167635287 @default.
• W4308248434 cites W2171744771 @default.
• W4308248434 cites W2237361821 @default.
• W4308248434 cites W2263773917 @default.
• W4308248434 cites W2344837005 @default.
• W4308248434 cites W2467852850 @default.
• W4308248434 cites W2474034009 @default.
• W4308248434 cites W2597993038 @default.
• W4308248434 cites W2605227686 @default.
• W4308248434 cites W2766689466 @default.
• W4308248434 cites W2788349473 @default.
• W4308248434 cites W2899005051 @default.
• W4308248434 cites W2949380767 @default.
• W4308248434 cites W2966693582 @default.
• W4308248434 cites W2975222635 @default.
• W4308248434 cites W3034270106 @default.
• W4308248434 cites W3046038707 @default.
• W4308248434 cites W3080992687 @default.
• W4308248434 cites W3096406960 @default.
• W4308248434 cites W3098092149 @default.
• W4308248434 cites W3098628468 @default.
• W4308248434 cites W3098728350 @default.
• W4308248434 cites W3098991679 @default.
• W4308248434 cites W3099240258 @default.
• W4308248434 cites W3099371412 @default.
• W4308248434 cites W3099536100 @default.
• W4308248434 cites W3099878876 @default.
• W4308248434 cites W3099950303 @default.
• W4308248434 cites W3100182684 @default.
• W4308248434 cites W3100215491 @default.
• W4308248434 cites W3100834105 @default.
• W4308248434 cites W3101020846 @default.
• W4308248434 cites W3102550802 @default.
• W4308248434 cites W3103177760 @default.
• W4308248434 cites W3104026304 @default.
• W4308248434 cites W3106292135 @default.
• W4308248434 cites W3106463647 @default.
• W4308248434 cites W3123632054 @default.
• W4308248434 cites W3134764504 @default.
• W4308248434 cites W3152670357 @default.
• W4308248434 cites W3177348811 @default.
• W4308248434 cites W3213147317 @default.
• W4308248434 cites W4200004652 @default.
• W4308248434 cites W4213259675 @default.
• W4308248434 cites W4220702124 @default.
• W4308248434 cites W4244945807 @default.
• W4308248434 cites W4280629988 @default.
• W4308248434 cites W4283079657 @default.
• W4308248434 cites W4289314799 @default.
• W4308248434 cites W4289919712 @default.
• W4308248434 cites W4290047213 @default.

• next