FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2892261218> ?p ?o ?g. }

• W2892261218 endingPage "4076" @default.
• W2892261218 startingPage "4058" @default.
• W2892261218 abstract "Recent observational studies of X-shaped structures revealed that values of their opening angles lie in a narrow range: from 20 deg to 43 deg with smaller X-shaped structures appearing to follow a characteristic opening angle ~ 27 deg - 31 deg. We use self-consistent numerical simulations to uncover what parameters of host galaxies govern the opening angle spread. We constructed a series of equilibrium models of galaxies with high spatial resolution, varying the dark halo and bulge contribution in the overall gravitational potential, the initial disc thickness of models and the Toomre parameter Q and followed their evolution for almost 8 Gyrs. Each model demonstrated the formation of clear X-structures with different flatness. We have obtained that opening angles lie in the range from 25 deg to 42 deg throughout the entire evolution. These values are roughly consistent with observational data. The greatest variation in the opening angles is obtained by varying the mass of the dark halo. The initial thickness of the disc and the Toomre parameter are responsible for smaller variations of the angle and shorter X-structures. An increase of both parameters changes the morphology of in-plane bars and X-structures. In some cases we observed even double X-structures. The main effect of the bulge is to prevent buckling at intermediate and late stages of the disc evolution. Comparison of models with different halo masses indicates that the smallest observable values of opening angles can be associated with the presence of a heavy dark halo (more than 3 masses of the disc within the optical radius)." @default.
• W2892261218 created "2018-09-27" @default.
• W2892261218 creator A5082126804 @default.
• W2892261218 creator A5088598560 @default.
• W2892261218 date "2018-09-29" @default.
• W2892261218 modified "2023-10-14" @default.
• W2892261218 title "What determines the flatness of X-shaped structures in edge-on galaxies?" @default.
• W2892261218 cites W1631788275 @default.
• W2892261218 cites W1965367046 @default.
• W2892261218 cites W1969586490 @default.
• W2892261218 cites W1978198015 @default.
• W2892261218 cites W1985631297 @default.
• W2892261218 cites W1988533866 @default.
• W2892261218 cites W2002253035 @default.
• W2892261218 cites W2007553814 @default.
• W2892261218 cites W2012780054 @default.
• W2892261218 cites W2014369477 @default.
• W2892261218 cites W2015050098 @default.
• W2892261218 cites W2018596526 @default.
• W2892261218 cites W2041542911 @default.
• W2892261218 cites W2046554872 @default.
• W2892261218 cites W2047117129 @default.
• W2892261218 cites W2059219979 @default.
• W2892261218 cites W2070675618 @default.
• W2892261218 cites W2084921690 @default.
• W2892261218 cites W2088205276 @default.
• W2892261218 cites W2095730734 @default.
• W2892261218 cites W2095943821 @default.
• W2892261218 cites W2104781956 @default.
• W2892261218 cites W2109606373 @default.
• W2892261218 cites W2114371196 @default.
• W2892261218 cites W2129685026 @default.
• W2892261218 cites W2148301921 @default.
• W2892261218 cites W2168235672 @default.
• W2892261218 cites W2171806185 @default.
• W2892261218 cites W2314476713 @default.
• W2892261218 cites W2559353449 @default.
• W2892261218 cites W2593651153 @default.
• W2892261218 cites W2735903034 @default.
• W2892261218 cites W2738501267 @default.
• W2892261218 cites W3098562365 @default.
• W2892261218 cites W3098779512 @default.
• W2892261218 cites W3099935024 @default.
• W2892261218 cites W3101004492 @default.
• W2892261218 cites W3101416702 @default.
• W2892261218 cites W3102017915 @default.
• W2892261218 cites W3102228877 @default.
• W2892261218 cites W3102706962 @default.
• W2892261218 cites W3102981450 @default.
• W2892261218 cites W3103772912 @default.
• W2892261218 cites W3103803516 @default.
• W2892261218 cites W3103877238 @default.
• W2892261218 cites W3104873233 @default.
• W2892261218 cites W3105542459 @default.
• W2892261218 cites W3105743869 @default.
• W2892261218 cites W3106439019 @default.
• W2892261218 cites W3106467243 @default.
• W2892261218 cites W3106475059 @default.
• W2892261218 cites W4289253600 @default.
• W2892261218 doi "https://doi.org/10.1093/mnras/sty2423" @default.
• W2892261218 hasPublicationYear "2018" @default.
• W2892261218 type Work @default.
• W2892261218 sameAs 2892261218 @default.
• W2892261218 citedByCount "14" @default.
• W2892261218 countsByYear W28922612182019 @default.
• W2892261218 countsByYear W28922612182020 @default.
• W2892261218 countsByYear W28922612182021 @default.
• W2892261218 countsByYear W28922612182022 @default.
• W2892261218 countsByYear W28922612182023 @default.
• W2892261218 crossrefType "journal-article" @default.
• W2892261218 hasAuthorship W2892261218A5082126804 @default.
• W2892261218 hasAuthorship W2892261218A5088598560 @default.
• W2892261218 hasBestOaLocation W28922612181 @default.
• W2892261218 hasConcept C10767094 @default.
• W2892261218 hasConcept C121332964 @default.
• W2892261218 hasConcept C159249277 @default.
• W2892261218 hasConcept C184665706 @default.
• W2892261218 hasConcept C26405456 @default.
• W2892261218 hasConcept C2778530986 @default.
• W2892261218 hasConcept C32848918 @default.
• W2892261218 hasConcept C44870925 @default.
• W2892261218 hasConcept C62520636 @default.
• W2892261218 hasConcept C88148261 @default.
• W2892261218 hasConcept C98444146 @default.
• W2892261218 hasConceptScore W2892261218C10767094 @default.
• W2892261218 hasConceptScore W2892261218C121332964 @default.
• W2892261218 hasConceptScore W2892261218C159249277 @default.
• W2892261218 hasConceptScore W2892261218C184665706 @default.
• W2892261218 hasConceptScore W2892261218C26405456 @default.
• W2892261218 hasConceptScore W2892261218C2778530986 @default.
• W2892261218 hasConceptScore W2892261218C32848918 @default.
• W2892261218 hasConceptScore W2892261218C44870925 @default.
• W2892261218 hasConceptScore W2892261218C62520636 @default.
• W2892261218 hasConceptScore W2892261218C88148261 @default.
• W2892261218 hasConceptScore W2892261218C98444146 @default.
• W2892261218 hasIssue "3" @default.
• W2892261218 hasLocation W28922612181 @default.
• W2892261218 hasLocation W28922612182 @default.

• next