Matches in SemOpenAlex for { <https://semopenalex.org/work/W1994418312> ?p ?o ?g. }
- W1994418312 endingPage "2064" @default.
- W1994418312 startingPage "2048" @default.
- W1994418312 abstract "We present a spectroscopic analysis based on measurements of two mainly age-dependent spectrophotometric indices in the 4000 Å rest-frame region, i.e. H+K(Ca ii) and Δ4000, for a sample of 15 early-type galaxies (ETGs) at 0.7 < zspec < 1.1, morphologically selected in the GOODS-South field. Ages derived from the two different indices by means of the comparison with stellar population synthesis models are not consistent with each other for at least nine galaxies (60 per cent of the sample), while for the remaining six galaxies, the ages derived from their global spectral energy distribution (SED) fitting are not consistent with those derived from the two indices. We then hypothesized that the stellar content of many galaxies is made of two stellar components with different ages. The double-component analysis, performed by taking into account both the index values and the observed SED, fully explains the observational data and improves the results of the standard one-component SED fitting in 9 out of the 15 objects, i.e. those for which the two indices point towards two different ages. In all of them, the bulk of the mass belongs to rather evolved stars, while a small mass fraction is many Gyr younger. In some cases, thanks to the sensitivity of the H+K(Ca ii) index, we find that the minor younger component reveals signs of recent star formation. The distribution of the ages of the younger stellar components appears uniformly in time and this suggests that small amounts of star formation could be common during the evolution of high-z ETGs. We argue the possibility that these new star formation episodes could be frequently triggered by internal causes due to the presence of small gas reservoir." @default.
- W1994418312 created "2016-06-24" @default.
- W1994418312 creator A5017962995 @default.
- W1994418312 creator A5055454821 @default.
- W1994418312 creator A5075295558 @default.
- W1994418312 creator A5079207976 @default.
- W1994418312 creator A5083337456 @default.
- W1994418312 date "2014-09-05" @default.
- W1994418312 modified "2023-09-23" @default.
- W1994418312 title "Spectral detection of multiple stellar populations in z ∼ 1 early-type galaxies" @default.
- W1994418312 cites W1529219299 @default.
- W1994418312 cites W1868671716 @default.
- W1994418312 cites W1963611021 @default.
- W1994418312 cites W1970356268 @default.
- W1994418312 cites W1973464280 @default.
- W1994418312 cites W1985370957 @default.
- W1994418312 cites W1994671833 @default.
- W1994418312 cites W2001085255 @default.
- W1994418312 cites W2004411957 @default.
- W1994418312 cites W2012886609 @default.
- W1994418312 cites W2017524870 @default.
- W1994418312 cites W2017719673 @default.
- W1994418312 cites W2020747414 @default.
- W1994418312 cites W2025020969 @default.
- W1994418312 cites W2026224376 @default.
- W1994418312 cites W2035808544 @default.
- W1994418312 cites W2040799945 @default.
- W1994418312 cites W2049852072 @default.
- W1994418312 cites W2054008190 @default.
- W1994418312 cites W2072289070 @default.
- W1994418312 cites W2108439497 @default.
- W1994418312 cites W2110846571 @default.
- W1994418312 cites W2115927937 @default.
- W1994418312 cites W2124511099 @default.
- W1994418312 cites W2138487987 @default.
- W1994418312 cites W2145106374 @default.
- W1994418312 cites W2147255867 @default.
- W1994418312 cites W2149739542 @default.
- W1994418312 cites W2151062050 @default.
- W1994418312 cites W2155026892 @default.
- W1994418312 cites W2952964124 @default.
- W1994418312 cites W3099020958 @default.
- W1994418312 cites W3099441451 @default.
- W1994418312 cites W3100024326 @default.
- W1994418312 cites W3102378148 @default.
- W1994418312 cites W3105233751 @default.
- W1994418312 cites W3115804805 @default.
- W1994418312 cites W3123116518 @default.
- W1994418312 cites W3123285458 @default.
- W1994418312 cites W3124028209 @default.
- W1994418312 cites W3124428178 @default.
- W1994418312 cites W3124734075 @default.
- W1994418312 cites W4235475162 @default.
- W1994418312 cites W4294589307 @default.
- W1994418312 cites W4297958636 @default.
- W1994418312 doi "https://doi.org/10.1093/mnras/stu1593" @default.
- W1994418312 hasPublicationYear "2014" @default.
- W1994418312 type Work @default.
- W1994418312 sameAs 1994418312 @default.
- W1994418312 citedByCount "21" @default.
- W1994418312 countsByYear W19944183122015 @default.
- W1994418312 countsByYear W19944183122016 @default.
- W1994418312 countsByYear W19944183122017 @default.
- W1994418312 countsByYear W19944183122018 @default.
- W1994418312 countsByYear W19944183122019 @default.
- W1994418312 countsByYear W19944183122022 @default.
- W1994418312 countsByYear W19944183122023 @default.
- W1994418312 crossrefType "journal-article" @default.
- W1994418312 hasAuthorship W1994418312A5017962995 @default.
- W1994418312 hasAuthorship W1994418312A5055454821 @default.
- W1994418312 hasAuthorship W1994418312A5075295558 @default.
- W1994418312 hasAuthorship W1994418312A5079207976 @default.
- W1994418312 hasAuthorship W1994418312A5083337456 @default.
- W1994418312 hasBestOaLocation W19944183121 @default.
- W1994418312 hasConcept C121332964 @default.
- W1994418312 hasConcept C125857072 @default.
- W1994418312 hasConcept C1276947 @default.
- W1994418312 hasConcept C144024400 @default.
- W1994418312 hasConcept C149923435 @default.
- W1994418312 hasConcept C150846664 @default.
- W1994418312 hasConcept C168589115 @default.
- W1994418312 hasConcept C2778623024 @default.
- W1994418312 hasConcept C2908647359 @default.
- W1994418312 hasConcept C42061751 @default.
- W1994418312 hasConcept C44870925 @default.
- W1994418312 hasConcept C4839761 @default.
- W1994418312 hasConcept C50425793 @default.
- W1994418312 hasConcept C98444146 @default.
- W1994418312 hasConceptScore W1994418312C121332964 @default.
- W1994418312 hasConceptScore W1994418312C125857072 @default.
- W1994418312 hasConceptScore W1994418312C1276947 @default.
- W1994418312 hasConceptScore W1994418312C144024400 @default.
- W1994418312 hasConceptScore W1994418312C149923435 @default.
- W1994418312 hasConceptScore W1994418312C150846664 @default.
- W1994418312 hasConceptScore W1994418312C168589115 @default.
- W1994418312 hasConceptScore W1994418312C2778623024 @default.
- W1994418312 hasConceptScore W1994418312C2908647359 @default.
- W1994418312 hasConceptScore W1994418312C42061751 @default.