Matches in SemOpenAlex for { <https://semopenalex.org/work/W3105097890> ?p ?o ?g. }
Showing items 1 to 92 of
92
with 100 items per page.
- W3105097890 endingPage "221" @default.
- W3105097890 startingPage "216" @default.
- W3105097890 abstract "Abstract We present a statistical analysis of the interactions between satellite galaxies in cosmological dark matter halos taken from fully self-consistent high-resolution simulations of galaxy clusters. We show that the number distribution of satellite encounters has a tail that extends to as many as three to four encounters per orbit. On average 30% of the substructure population had at least one encounter (per orbit) with another satellite galaxy. However, this result depends on the age of the dark matter host halo with a clear trend for more interactions in younger systems. We also report a correlation between the number of encounters and the distance of the satellites to the centre of the cluster — satellite galaxies closer to the centre experience more interactions. However, this can be simply explained by the radial distribution of the substructure population and merely reflects the fact that the density of satellites is higher in those regions. In order to find substructure galaxies we applied (and present) a new technique based upon the N -body code MLAPM. This new halo finder MHF (MLAPM’s halo finder) acts with exactly the same accuracy as the N -body code itself and is therefore free of any bias and spurious mismatch between simulation data and halo finding precision related to numerical effects." @default.
- W3105097890 created "2020-11-23" @default.
- W3105097890 creator A5026840193 @default.
- W3105097890 creator A5076755949 @default.
- W3105097890 creator A5089236888 @default.
- W3105097890 date "2004-01-01" @default.
- W3105097890 modified "2023-10-16" @default.
- W3105097890 title "Interactions of Satellite Galaxies in Cosmological Dark Matter Halos" @default.
- W3105097890 cites W1968412179 @default.
- W3105097890 cites W1974309328 @default.
- W3105097890 cites W1978511078 @default.
- W3105097890 cites W1993132186 @default.
- W3105097890 cites W1999367759 @default.
- W3105097890 cites W2032469582 @default.
- W3105097890 cites W2032728617 @default.
- W3105097890 cites W2066207788 @default.
- W3105097890 cites W2068306188 @default.
- W3105097890 cites W2098776230 @default.
- W3105097890 cites W2110854340 @default.
- W3105097890 cites W2118265220 @default.
- W3105097890 cites W2121394747 @default.
- W3105097890 cites W2139031955 @default.
- W3105097890 cites W2154542873 @default.
- W3105097890 cites W3099361836 @default.
- W3105097890 cites W3105140539 @default.
- W3105097890 doi "https://doi.org/10.1071/as04018" @default.
- W3105097890 hasPublicationYear "2004" @default.
- W3105097890 type Work @default.
- W3105097890 sameAs 3105097890 @default.
- W3105097890 citedByCount "9" @default.
- W3105097890 countsByYear W31050978902019 @default.
- W3105097890 countsByYear W31050978902023 @default.
- W3105097890 crossrefType "journal-article" @default.
- W3105097890 hasAuthorship W3105097890A5026840193 @default.
- W3105097890 hasAuthorship W3105097890A5076755949 @default.
- W3105097890 hasAuthorship W3105097890A5089236888 @default.
- W3105097890 hasBestOaLocation W31050978901 @default.
- W3105097890 hasConcept C113789861 @default.
- W3105097890 hasConcept C121332964 @default.
- W3105097890 hasConcept C127413603 @default.
- W3105097890 hasConcept C1276947 @default.
- W3105097890 hasConcept C144024400 @default.
- W3105097890 hasConcept C149923435 @default.
- W3105097890 hasConcept C159249277 @default.
- W3105097890 hasConcept C174802034 @default.
- W3105097890 hasConcept C184665706 @default.
- W3105097890 hasConcept C2908647359 @default.
- W3105097890 hasConcept C44870925 @default.
- W3105097890 hasConcept C51650839 @default.
- W3105097890 hasConcept C66938386 @default.
- W3105097890 hasConcept C68447186 @default.
- W3105097890 hasConcept C88148261 @default.
- W3105097890 hasConcept C98444146 @default.
- W3105097890 hasConcept C99679407 @default.
- W3105097890 hasConceptScore W3105097890C113789861 @default.
- W3105097890 hasConceptScore W3105097890C121332964 @default.
- W3105097890 hasConceptScore W3105097890C127413603 @default.
- W3105097890 hasConceptScore W3105097890C1276947 @default.
- W3105097890 hasConceptScore W3105097890C144024400 @default.
- W3105097890 hasConceptScore W3105097890C149923435 @default.
- W3105097890 hasConceptScore W3105097890C159249277 @default.
- W3105097890 hasConceptScore W3105097890C174802034 @default.
- W3105097890 hasConceptScore W3105097890C184665706 @default.
- W3105097890 hasConceptScore W3105097890C2908647359 @default.
- W3105097890 hasConceptScore W3105097890C44870925 @default.
- W3105097890 hasConceptScore W3105097890C51650839 @default.
- W3105097890 hasConceptScore W3105097890C66938386 @default.
- W3105097890 hasConceptScore W3105097890C68447186 @default.
- W3105097890 hasConceptScore W3105097890C88148261 @default.
- W3105097890 hasConceptScore W3105097890C98444146 @default.
- W3105097890 hasConceptScore W3105097890C99679407 @default.
- W3105097890 hasIssue "2" @default.
- W3105097890 hasLocation W31050978901 @default.
- W3105097890 hasOpenAccess W3105097890 @default.
- W3105097890 hasPrimaryLocation W31050978901 @default.
- W3105097890 hasRelatedWork W1868070316 @default.
- W3105097890 hasRelatedWork W1994483112 @default.
- W3105097890 hasRelatedWork W3104369048 @default.
- W3105097890 hasRelatedWork W3105097890 @default.
- W3105097890 hasRelatedWork W3105129797 @default.
- W3105097890 hasRelatedWork W3122666341 @default.
- W3105097890 hasRelatedWork W3168650543 @default.
- W3105097890 hasRelatedWork W4226441121 @default.
- W3105097890 hasRelatedWork W4294604595 @default.
- W3105097890 hasRelatedWork W4379538533 @default.
- W3105097890 hasVolume "21" @default.
- W3105097890 isParatext "false" @default.
- W3105097890 isRetracted "false" @default.
- W3105097890 magId "3105097890" @default.
- W3105097890 workType "article" @default.