FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1892049369> ?p ?o ?g. }

• W1892049369 endingPage "644" @default.
• W1892049369 startingPage "625" @default.
• W1892049369 abstract "We present a detailed surface density analysis of a large sample of simulated collisionless mergers of disc galaxies with bulges (mass ratios 1:1, 2:1, 3:1, 4:1 and 6:1) and without bulges (mass ratios 1:1 and 3:1). A dissipative component was not included. The randomly projected remnants were fit with a single Sérsic function and a Sérsic function plus an exponential. They were classified, according to their bulge-to-total (B/T) ratio, either as a one-component system or as a two-component system. In general, projection effects change the classification of a remnant. Only merger remnants of discs with bulges show properties similar to observed early-type galaxies. Their B/T ratios are in the range 0.2 < B/T < 1. Surprisingly, the initial mass ratio has a weak influence on the distributions of B/T, effective radius and Sérsic index n. For all one-component projections (≈60 per cent of all projections), the Sérsic index distribution peaks at 3 < n < 4. However, the mass ratio is tightly linked to the properties of the outer exponential components which resemble pressure-supported, spheroidal haloes for 1:1 and 2:1 remnants and elongated heated discs for 6:1 remnants. We found distinct correlations between the fitting parameters which are very similar to observed relations (e.g. larger bulges have lower effective surface densities). No indications for a correlation between the surface density profiles and other global parameters like remnant masses, isophotal shapes or central velocity dispersions are found. The remnants have properties similar to giant elliptical galaxies in the intermediate-mass regime. A binary disc merger origin for all early-type galaxies, especially the most massive ones, is unlikely. Observed nearby merger remnants have properties similar to the simulated remnants. They can have formed from binary disc mergers and might evolve into early-type galaxies within a few Gyr." @default.
• W1892049369 created "2016-06-24" @default.
• W1892049369 creator A5022575311 @default.
• W1892049369 creator A5026933127 @default.
• W1892049369 date "2006-05-18" @default.
• W1892049369 modified "2023-10-03" @default.
• W1892049369 title "Surface density profiles of collisionless disc merger remnants" @default.
• W1892049369 cites W1657761426 @default.
• W1892049369 cites W1676521865 @default.
• W1892049369 cites W1966665981 @default.
• W1892049369 cites W1972478821 @default.
• W1892049369 cites W1972867229 @default.
• W1892049369 cites W1975889665 @default.
• W1892049369 cites W1978219874 @default.
• W1892049369 cites W1980407182 @default.
• W1892049369 cites W1981189137 @default.
• W1892049369 cites W1983915830 @default.
• W1892049369 cites W1987799421 @default.
• W1892049369 cites W1993839984 @default.
• W1892049369 cites W1994837005 @default.
• W1892049369 cites W1995341836 @default.
• W1892049369 cites W1999793606 @default.
• W1892049369 cites W2001717952 @default.
• W1892049369 cites W2012733001 @default.
• W1892049369 cites W2015130027 @default.
• W1892049369 cites W2016226934 @default.
• W1892049369 cites W2022375968 @default.
• W1892049369 cites W2030326695 @default.
• W1892049369 cites W2031800963 @default.
• W1892049369 cites W2037816996 @default.
• W1892049369 cites W2040459248 @default.
• W1892049369 cites W2041542911 @default.
• W1892049369 cites W2044871593 @default.
• W1892049369 cites W2046443312 @default.
• W1892049369 cites W2051313615 @default.
• W1892049369 cites W2060448616 @default.
• W1892049369 cites W2062369951 @default.
• W1892049369 cites W2086332505 @default.
• W1892049369 cites W2086949239 @default.
• W1892049369 cites W2088833158 @default.
• W1892049369 cites W2098666281 @default.
• W1892049369 cites W2110417064 @default.
• W1892049369 cites W2110487529 @default.
• W1892049369 cites W2117201920 @default.
• W1892049369 cites W2132898393 @default.
• W1892049369 cites W2138374703 @default.
• W1892049369 cites W2145710642 @default.
• W1892049369 cites W2154955582 @default.
• W1892049369 cites W2156690198 @default.
• W1892049369 cites W2159354593 @default.
• W1892049369 cites W3099006964 @default.
• W1892049369 cites W3099118016 @default.
• W1892049369 cites W3099886821 @default.
• W1892049369 cites W3099907295 @default.
• W1892049369 cites W3099982585 @default.
• W1892049369 cites W3101809885 @default.
• W1892049369 cites W3101988252 @default.
• W1892049369 cites W3102023246 @default.
• W1892049369 cites W3103262655 @default.
• W1892049369 cites W3103899138 @default.
• W1892049369 cites W3103987558 @default.
• W1892049369 cites W3104796515 @default.
• W1892049369 cites W3105450836 @default.
• W1892049369 cites W3106085136 @default.
• W1892049369 cites W3106258903 @default.
• W1892049369 cites W3125145960 @default.
• W1892049369 cites W3169916273 @default.
• W1892049369 doi "https://doi.org/10.1111/j.1365-2966.2006.10252.x" @default.
• W1892049369 hasPublicationYear "2006" @default.
• W1892049369 type Work @default.
• W1892049369 sameAs 1892049369 @default.
• W1892049369 citedByCount "115" @default.
• W1892049369 countsByYear W18920493692012 @default.
• W1892049369 countsByYear W18920493692013 @default.
• W1892049369 countsByYear W18920493692014 @default.
• W1892049369 countsByYear W18920493692015 @default.
• W1892049369 countsByYear W18920493692016 @default.
• W1892049369 countsByYear W18920493692018 @default.
• W1892049369 countsByYear W18920493692019 @default.
• W1892049369 countsByYear W18920493692020 @default.
• W1892049369 countsByYear W18920493692021 @default.
• W1892049369 countsByYear W18920493692022 @default.
• W1892049369 countsByYear W18920493692023 @default.
• W1892049369 crossrefType "journal-article" @default.
• W1892049369 hasAuthorship W1892049369A5022575311 @default.
• W1892049369 hasAuthorship W1892049369A5026933127 @default.
• W1892049369 hasBestOaLocation W18920493691 @default.
• W1892049369 hasConcept C10767094 @default.
• W1892049369 hasConcept C121332964 @default.
• W1892049369 hasConcept C127529279 @default.
• W1892049369 hasConcept C134306372 @default.
• W1892049369 hasConcept C151376022 @default.
• W1892049369 hasConcept C178635117 @default.
• W1892049369 hasConcept C188232333 @default.
• W1892049369 hasConcept C33923547 @default.
• W1892049369 hasConcept C38652104 @default.
• W1892049369 hasConcept C41008148 @default.
• W1892049369 hasConcept C44870925 @default.

• next