Matches in SemOpenAlex for { <https://semopenalex.org/work/W2892013438> ?p ?o ?g. }
- W2892013438 abstract "We study the shape and evolution of the star formation main sequence in three independently developed semi-analytic models of galaxy formation. We focus, in particular, on the characterization of the model galaxies that are significantly above the main sequence, and that can be identified with galaxies classified as `starburst' in recent observational work. We find that, in all three models considered, star formation triggered by merger events (both minor and major) contribute to only a very small fraction of the cosmic density of star formation. While mergers are associated to bursts of star formation in all models, galaxies that experienced recent merger events are not necessarily significantly above the main sequence. On the other hand, `starburst galaxies' are not necessarily associated with merger episodes, especially at the low-mass end. Galaxies that experienced recent mergers can have relatively low levels of star formation when/if the merger is gas-poor, and galaxies with no recent merger can experience episodes of starbursts due to a combination of large amount of cold gas available from cooling/accretion events and/or small disk radii which increases the cold gas surface density." @default.
- W2892013438 created "2018-09-27" @default.
- W2892013438 creator A5027633831 @default.
- W2892013438 creator A5028859676 @default.
- W2892013438 creator A5091006390 @default.
- W2892013438 creator A5091335146 @default.
- W2892013438 date "2018-11-06" @default.
- W2892013438 modified "2023-09-25" @default.
- W2892013438 title "Starburst galaxies in semi-analytic models of galaxy formation and evolution" @default.
- W2892013438 cites W1724036414 @default.
- W2892013438 cites W1929217367 @default.
- W2892013438 cites W1963831836 @default.
- W2892013438 cites W1964055719 @default.
- W2892013438 cites W1972901985 @default.
- W2892013438 cites W1977843574 @default.
- W2892013438 cites W1985814919 @default.
- W2892013438 cites W1994968723 @default.
- W2892013438 cites W1996169450 @default.
- W2892013438 cites W1997662069 @default.
- W2892013438 cites W1999046479 @default.
- W2892013438 cites W2034241894 @default.
- W2892013438 cites W2037816996 @default.
- W2892013438 cites W2049524691 @default.
- W2892013438 cites W2049698250 @default.
- W2892013438 cites W2082012530 @default.
- W2892013438 cites W2086328762 @default.
- W2892013438 cites W2090459210 @default.
- W2892013438 cites W2109146631 @default.
- W2892013438 cites W2116466430 @default.
- W2892013438 cites W2120523711 @default.
- W2892013438 cites W2125977823 @default.
- W2892013438 cites W2132646102 @default.
- W2892013438 cites W2133810750 @default.
- W2892013438 cites W2141709306 @default.
- W2892013438 cites W2150995848 @default.
- W2892013438 cites W2155315054 @default.
- W2892013438 cites W2166365370 @default.
- W2892013438 cites W2167388685 @default.
- W2892013438 cites W2169439142 @default.
- W2892013438 cites W2171992101 @default.
- W2892013438 cites W2208450685 @default.
- W2892013438 cites W2258390913 @default.
- W2892013438 cites W2531463523 @default.
- W2892013438 cites W2607270102 @default.
- W2892013438 cites W2807009254 @default.
- W2892013438 cites W2810658404 @default.
- W2892013438 cites W2953228579 @default.
- W2892013438 cites W2963597745 @default.
- W2892013438 cites W2963779394 @default.
- W2892013438 cites W2964219748 @default.
- W2892013438 cites W3099149995 @default.
- W2892013438 cites W3099471130 @default.
- W2892013438 cites W3099575261 @default.
- W2892013438 cites W3099640725 @default.
- W2892013438 cites W3100527122 @default.
- W2892013438 cites W3100971600 @default.
- W2892013438 cites W3101136979 @default.
- W2892013438 cites W3101735292 @default.
- W2892013438 cites W3102834807 @default.
- W2892013438 cites W3104728800 @default.
- W2892013438 cites W3105161400 @default.
- W2892013438 cites W3106418973 @default.
- W2892013438 cites W3121560983 @default.
- W2892013438 cites W3122003039 @default.
- W2892013438 cites W3124349042 @default.
- W2892013438 cites W4213122534 @default.
- W2892013438 doi "https://doi.org/10.1093/mnras/sty2998" @default.
- W2892013438 hasPublicationYear "2018" @default.
- W2892013438 type Work @default.
- W2892013438 sameAs 2892013438 @default.
- W2892013438 citedByCount "6" @default.
- W2892013438 countsByYear W28920134382019 @default.
- W2892013438 countsByYear W28920134382021 @default.
- W2892013438 countsByYear W28920134382022 @default.
- W2892013438 crossrefType "journal-article" @default.
- W2892013438 hasAuthorship W2892013438A5027633831 @default.
- W2892013438 hasAuthorship W2892013438A5028859676 @default.
- W2892013438 hasAuthorship W2892013438A5091006390 @default.
- W2892013438 hasAuthorship W2892013438A5091335146 @default.
- W2892013438 hasBestOaLocation W28920134382 @default.
- W2892013438 hasConcept C121332964 @default.
- W2892013438 hasConcept C125857072 @default.
- W2892013438 hasConcept C1276947 @default.
- W2892013438 hasConcept C134122466 @default.
- W2892013438 hasConcept C165641701 @default.
- W2892013438 hasConcept C174802034 @default.
- W2892013438 hasConcept C205327720 @default.
- W2892013438 hasConcept C2776401274 @default.
- W2892013438 hasConcept C44870925 @default.
- W2892013438 hasConcept C871022 @default.
- W2892013438 hasConcept C89108925 @default.
- W2892013438 hasConcept C98444146 @default.
- W2892013438 hasConceptScore W2892013438C121332964 @default.
- W2892013438 hasConceptScore W2892013438C125857072 @default.
- W2892013438 hasConceptScore W2892013438C1276947 @default.
- W2892013438 hasConceptScore W2892013438C134122466 @default.
- W2892013438 hasConceptScore W2892013438C165641701 @default.
- W2892013438 hasConceptScore W2892013438C174802034 @default.
- W2892013438 hasConceptScore W2892013438C205327720 @default.
- W2892013438 hasConceptScore W2892013438C2776401274 @default.