Matches in SemOpenAlex for { <https://semopenalex.org/work/W2152671803> ?p ?o ?g. }
- W2152671803 endingPage "668" @default.
- W2152671803 startingPage "655" @default.
- W2152671803 abstract "We have investigated the poorly-understood origin of nitrogen in the early Galaxy by determining N abundances in 35 extremely metal-poor halo giants (22 stars have [Fe/H]<-3.0) using the C and O abundances determined in Paper V. Because any dredge-up of CNO processed material to the surface may complicate the interpretation of CNO abundances in giants, we have also measured the surface abundance of lithium. Our sample shows a clear dichotomy between two groups of stars. The first group shows evidence of C to N conversion through CN cycling and strong Li dilution, a signature of mixing. The second group shows no evidence for C to N conversion, and Li is only moderately diluted, and we conclude that their C and N abundances are very close to those of the gas from which they formed in the early Galaxy. These unmixed stars reflect the abundances in the early Galaxy: the [C/Fe] ratio is constant (about +0.2 dex) and the [C/Mg] ratio is close to solar at low metallicity, favouring a high C production by massive zero-metal supernovae. The [N/Fe] and [N/Mg] ratios scatter widely. The larger values of these ratios define a flat upper plateau ([N/Mg]= 0.0, [N/Fe]= +0.1), which could reflect higher values within a wide range of yields of zero-metal Sne II. Alternatively, by analogy with the DLA's, the lower abundances ([N/Mg]= -1.1, [N/Fe]= -0.7) could reflect generally low yields from the first Sne II, the other stars being N enhanced by winds of massive Asymptotic Giant Branch (AGB) stars. At present it cannot be decided whether primary N is produced primarily in SNe II or in massive AGB stars, or in both. The stellar N abundances and [N/O] ratios are compatible with those found in Damped Lyman-alpha (DLA) systems." @default.
- W2152671803 created "2016-06-24" @default.
- W2152671803 creator A5001288481 @default.
- W2152671803 creator A5004372939 @default.
- W2152671803 creator A5007399893 @default.
- W2152671803 creator A5008849198 @default.
- W2152671803 creator A5011711480 @default.
- W2152671803 creator A5019716342 @default.
- W2152671803 creator A5026091792 @default.
- W2152671803 creator A5031906583 @default.
- W2152671803 creator A5046801184 @default.
- W2152671803 creator A5051848532 @default.
- W2152671803 creator A5065682440 @default.
- W2152671803 creator A5066363499 @default.
- W2152671803 creator A5073780419 @default.
- W2152671803 creator A5088719533 @default.
- W2152671803 date "2005-01-20" @default.
- W2152671803 modified "2023-10-11" @default.
- W2152671803 title "First stars VI – Abundances of C, N, O, Li, and mixing in extremely metal-poor giants. Galactic evolution of the light elements" @default.
- W2152671803 cites W1556334824 @default.
- W2152671803 cites W1634072782 @default.
- W2152671803 cites W1659875532 @default.
- W2152671803 cites W1680174945 @default.
- W2152671803 cites W1966487744 @default.
- W2152671803 cites W1977335790 @default.
- W2152671803 cites W1979257798 @default.
- W2152671803 cites W2009489905 @default.
- W2152671803 cites W2012108819 @default.
- W2152671803 cites W2016846163 @default.
- W2152671803 cites W2016874768 @default.
- W2152671803 cites W2020215161 @default.
- W2152671803 cites W2029384527 @default.
- W2152671803 cites W2029990291 @default.
- W2152671803 cites W2031387259 @default.
- W2152671803 cites W2043258333 @default.
- W2152671803 cites W2059519221 @default.
- W2152671803 cites W2073332494 @default.
- W2152671803 cites W2081260751 @default.
- W2152671803 cites W2083805862 @default.
- W2152671803 cites W2085689196 @default.
- W2152671803 cites W2089583403 @default.
- W2152671803 cites W2093813575 @default.
- W2152671803 cites W2103024508 @default.
- W2152671803 cites W2106402956 @default.
- W2152671803 cites W2119855645 @default.
- W2152671803 cites W2128490266 @default.
- W2152671803 cites W2139006073 @default.
- W2152671803 cites W2139594802 @default.
- W2152671803 cites W2144431664 @default.
- W2152671803 cites W2161137739 @default.
- W2152671803 cites W2166193059 @default.
- W2152671803 cites W3021727832 @default.
- W2152671803 cites W3095204031 @default.
- W2152671803 cites W3098397727 @default.
- W2152671803 cites W3100331031 @default.
- W2152671803 cites W3101930143 @default.
- W2152671803 cites W3106327613 @default.
- W2152671803 cites W3106419190 @default.
- W2152671803 cites W4244945807 @default.
- W2152671803 cites W4301332103 @default.
- W2152671803 doi "https://doi.org/10.1051/0004-6361:20041274" @default.
- W2152671803 hasPublicationYear "2005" @default.
- W2152671803 type Work @default.
- W2152671803 sameAs 2152671803 @default.
- W2152671803 citedByCount "347" @default.
- W2152671803 countsByYear W21526718032012 @default.
- W2152671803 countsByYear W21526718032013 @default.
- W2152671803 countsByYear W21526718032014 @default.
- W2152671803 countsByYear W21526718032015 @default.
- W2152671803 countsByYear W21526718032016 @default.
- W2152671803 countsByYear W21526718032017 @default.
- W2152671803 countsByYear W21526718032018 @default.
- W2152671803 countsByYear W21526718032019 @default.
- W2152671803 countsByYear W21526718032020 @default.
- W2152671803 countsByYear W21526718032021 @default.
- W2152671803 countsByYear W21526718032022 @default.
- W2152671803 countsByYear W21526718032023 @default.
- W2152671803 crossrefType "journal-article" @default.
- W2152671803 hasAuthorship W2152671803A5001288481 @default.
- W2152671803 hasAuthorship W2152671803A5004372939 @default.
- W2152671803 hasAuthorship W2152671803A5007399893 @default.
- W2152671803 hasAuthorship W2152671803A5008849198 @default.
- W2152671803 hasAuthorship W2152671803A5011711480 @default.
- W2152671803 hasAuthorship W2152671803A5019716342 @default.
- W2152671803 hasAuthorship W2152671803A5026091792 @default.
- W2152671803 hasAuthorship W2152671803A5031906583 @default.
- W2152671803 hasAuthorship W2152671803A5046801184 @default.
- W2152671803 hasAuthorship W2152671803A5051848532 @default.
- W2152671803 hasAuthorship W2152671803A5065682440 @default.
- W2152671803 hasAuthorship W2152671803A5066363499 @default.
- W2152671803 hasAuthorship W2152671803A5073780419 @default.
- W2152671803 hasAuthorship W2152671803A5088719533 @default.
- W2152671803 hasBestOaLocation W21526718031 @default.
- W2152671803 hasConcept C121332964 @default.
- W2152671803 hasConcept C127592171 @default.
- W2152671803 hasConcept C150846664 @default.
- W2152671803 hasConcept C174802034 @default.
- W2152671803 hasConcept C178790620 @default.