FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1985209384> ?p ?o ?g. }

• W1985209384 endingPage "5" @default.
• W1985209384 startingPage "5" @default.
• W1985209384 abstract "We present for the first time metallicity maps generated using data from the Wide Field Spectrograph (WiFeS) on the ANU 2.3m of 9 Luminous Infrared Galaxies (LIRGs) and discuss the abundance gradients and distribution of metals in these systems. We have carried out optical integral field spectroscopy (IFS) of several several LIRGs in various merger phases to investigate the merger process. In a major merger of two spiral galaxies with preexisting disk abundance gradients, the changing distribution of metals can be used as a tracer of gas flows in the merging system as low metallicity gas is transported from the outskirts of each galaxy to their nuclei. We employ this fact to probe merger properties by using the emission lines in our IFS data to calculate the gas-phase metallicity in each system. We create abundance maps and subsequently derive a metallicity gradient from each map. We compare our measured gradients to merger stage as well as several possible tracers of merger progress and observed nuclear abundances. We discuss our work in the context of previous abundance gradient observations and compare our results to new galaxy merger models which trace metallicity gradient. Our results agree with the observed flattening of metallicity gradients as a merger progresses. We compare our results with new theoretical predictions that include chemical enrichment. Our data show remarkable agreement with these simulations." @default.
• W1985209384 created "2016-06-24" @default.
• W1985209384 creator A5027796962 @default.
• W1985209384 creator A5033229802 @default.
• W1985209384 creator A5056544280 @default.
• W1985209384 creator A5066048279 @default.
• W1985209384 creator A5085246344 @default.
• W1985209384 date "2012-06-07" @default.
• W1985209384 modified "2023-10-18" @default.
• W1985209384 title "AN INTEGRAL FIELD STUDY OF ABUNDANCE GRADIENTS IN NEARBY LUMINOUS INFRARED GALAXIES" @default.
• W1985209384 cites W1980940672 @default.
• W1985209384 cites W1989738732 @default.
• W1985209384 cites W1992570077 @default.
• W1985209384 cites W1993166397 @default.
• W1985209384 cites W1997015919 @default.
• W1985209384 cites W2007741717 @default.
• W1985209384 cites W2010356064 @default.
• W1985209384 cites W2012759655 @default.
• W1985209384 cites W2023585815 @default.
• W1985209384 cites W2046620005 @default.
• W1985209384 cites W2048398007 @default.
• W1985209384 cites W2067857092 @default.
• W1985209384 cites W2069847092 @default.
• W1985209384 cites W2071933657 @default.
• W1985209384 cites W2090135680 @default.
• W1985209384 cites W2091010926 @default.
• W1985209384 cites W2096147217 @default.
• W1985209384 cites W2104302651 @default.
• W1985209384 cites W2109466814 @default.
• W1985209384 cites W2128904482 @default.
• W1985209384 cites W2144334431 @default.
• W1985209384 cites W3099142252 @default.
• W1985209384 cites W3099674141 @default.
• W1985209384 cites W3102076853 @default.
• W1985209384 cites W3102865120 @default.
• W1985209384 cites W3103933065 @default.
• W1985209384 cites W3128285573 @default.
• W1985209384 doi "https://doi.org/10.1088/0004-637x/753/1/5" @default.
• W1985209384 hasPublicationYear "2012" @default.
• W1985209384 type Work @default.
• W1985209384 sameAs 1985209384 @default.
• W1985209384 citedByCount "102" @default.
• W1985209384 countsByYear W19852093842012 @default.
• W1985209384 countsByYear W19852093842013 @default.
• W1985209384 countsByYear W19852093842014 @default.
• W1985209384 countsByYear W19852093842015 @default.
• W1985209384 countsByYear W19852093842016 @default.
• W1985209384 countsByYear W19852093842017 @default.
• W1985209384 countsByYear W19852093842018 @default.
• W1985209384 countsByYear W19852093842019 @default.
• W1985209384 countsByYear W19852093842020 @default.
• W1985209384 countsByYear W19852093842021 @default.
• W1985209384 countsByYear W19852093842022 @default.
• W1985209384 countsByYear W19852093842023 @default.
• W1985209384 crossrefType "journal-article" @default.
• W1985209384 hasAuthorship W1985209384A5027796962 @default.
• W1985209384 hasAuthorship W1985209384A5033229802 @default.
• W1985209384 hasAuthorship W1985209384A5056544280 @default.
• W1985209384 hasAuthorship W1985209384A5066048279 @default.
• W1985209384 hasAuthorship W1985209384A5085246344 @default.
• W1985209384 hasBestOaLocation W19852093841 @default.
• W1985209384 hasConcept C121332964 @default.
• W1985209384 hasConcept C1276947 @default.
• W1985209384 hasConcept C151730666 @default.
• W1985209384 hasConcept C174802034 @default.
• W1985209384 hasConcept C19444555 @default.
• W1985209384 hasConcept C2779343474 @default.
• W1985209384 hasConcept C44870925 @default.
• W1985209384 hasConcept C505870484 @default.
• W1985209384 hasConcept C63585750 @default.
• W1985209384 hasConcept C77077793 @default.
• W1985209384 hasConcept C86803240 @default.
• W1985209384 hasConcept C89108925 @default.
• W1985209384 hasConcept C98444146 @default.
• W1985209384 hasConcept C99465377 @default.
• W1985209384 hasConceptScore W1985209384C121332964 @default.
• W1985209384 hasConceptScore W1985209384C1276947 @default.
• W1985209384 hasConceptScore W1985209384C151730666 @default.
• W1985209384 hasConceptScore W1985209384C174802034 @default.
• W1985209384 hasConceptScore W1985209384C19444555 @default.
• W1985209384 hasConceptScore W1985209384C2779343474 @default.
• W1985209384 hasConceptScore W1985209384C44870925 @default.
• W1985209384 hasConceptScore W1985209384C505870484 @default.
• W1985209384 hasConceptScore W1985209384C63585750 @default.
• W1985209384 hasConceptScore W1985209384C77077793 @default.
• W1985209384 hasConceptScore W1985209384C86803240 @default.
• W1985209384 hasConceptScore W1985209384C89108925 @default.
• W1985209384 hasConceptScore W1985209384C98444146 @default.
• W1985209384 hasConceptScore W1985209384C99465377 @default.
• W1985209384 hasIssue "1" @default.
• W1985209384 hasLocation W19852093841 @default.
• W1985209384 hasLocation W19852093842 @default.
• W1985209384 hasOpenAccess W1985209384 @default.
• W1985209384 hasPrimaryLocation W19852093841 @default.
• W1985209384 hasRelatedWork W1825301338 @default.
• W1985209384 hasRelatedWork W1922699913 @default.
• W1985209384 hasRelatedWork W2159148367 @default.
• W1985209384 hasRelatedWork W2168587750 @default.

• next