FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3099681195> ?p ?o ?g. }

• W3099681195 endingPage "914" @default.
• W3099681195 startingPage "907" @default.
• W3099681195 abstract "We consider the dynamical evolution of a disk of stars orbiting a central black hole. In particular, we focus on the effect of the stellar mass function on the evolution of the disk, using both analytic arguments and numerical simulations. We apply our model to the ring of massive stars at ≃0.1 pc from the Galactic center, assuming that the stars formed in a cold, circular disk, and find that our model requires the presence of a significant population of massive (>100 M☉) stars in order to explain the observed eccentricities of 0.2-0.3. Moreover, in order to limit the damping of the heavier stars' eccentricities, we also require fewer low-mass stars than expected from a Salpeter mass function, giving strong evidence for a significantly top-heavy mass function in the rings of stars seen near to the Galactic center. We also note that the maximum possible eccentricities attainable from circular initial conditions at ages of <10 Myr are around 0.4-0.5, and we suggest that any rings of stars found with higher eccentricities were probably not formed from circular disks." @default.
• W3099681195 created "2020-11-23" @default.
• W3099681195 creator A5043144883 @default.
• W3099681195 creator A5069079061 @default.
• W3099681195 creator A5085223431 @default.
• W3099681195 date "2007-01-10" @default.
• W3099681195 modified "2023-10-16" @default.
• W3099681195 title "Constraints on the Stellar Mass Function from Stellar Dynamics at the Galactic Center" @default.
• W3099681195 cites W1965697852 @default.
• W3099681195 cites W1992587034 @default.
• W3099681195 cites W2003387896 @default.
• W3099681195 cites W2010269252 @default.
• W3099681195 cites W2011369346 @default.
• W3099681195 cites W2014299735 @default.
• W3099681195 cites W2017466075 @default.
• W3099681195 cites W2019594817 @default.
• W3099681195 cites W2030776989 @default.
• W3099681195 cites W2054373355 @default.
• W3099681195 cites W2058064642 @default.
• W3099681195 cites W2065575055 @default.
• W3099681195 cites W2090568902 @default.
• W3099681195 cites W2091529942 @default.
• W3099681195 cites W2106449774 @default.
• W3099681195 cites W2116412082 @default.
• W3099681195 cites W2123710893 @default.
• W3099681195 cites W2124832126 @default.
• W3099681195 cites W2139187938 @default.
• W3099681195 cites W2140490206 @default.
• W3099681195 cites W2157058681 @default.
• W3099681195 cites W2948909576 @default.
• W3099681195 cites W2951376817 @default.
• W3099681195 cites W2990193255 @default.
• W3099681195 cites W3017243433 @default.
• W3099681195 cites W3098258833 @default.
• W3099681195 cites W3098279946 @default.
• W3099681195 cites W3100241463 @default.
• W3099681195 cites W3100631228 @default.
• W3099681195 cites W3102424143 @default.
• W3099681195 cites W3105932956 @default.
• W3099681195 cites W3123522961 @default.
• W3099681195 cites W3124301469 @default.
• W3099681195 cites W3176148648 @default.
• W3099681195 cites W4251585788 @default.
• W3099681195 doi "https://doi.org/10.1086/509709" @default.
• W3099681195 hasPublicationYear "2007" @default.
• W3099681195 type Work @default.
• W3099681195 sameAs 3099681195 @default.
• W3099681195 citedByCount "48" @default.
• W3099681195 countsByYear W30996811952012 @default.
• W3099681195 countsByYear W30996811952013 @default.
• W3099681195 countsByYear W30996811952014 @default.
• W3099681195 countsByYear W30996811952015 @default.
• W3099681195 countsByYear W30996811952016 @default.
• W3099681195 countsByYear W30996811952017 @default.
• W3099681195 countsByYear W30996811952018 @default.
• W3099681195 countsByYear W30996811952020 @default.
• W3099681195 countsByYear W30996811952021 @default.
• W3099681195 countsByYear W30996811952022 @default.
• W3099681195 countsByYear W30996811952023 @default.
• W3099681195 crossrefType "journal-article" @default.
• W3099681195 hasAuthorship W3099681195A5043144883 @default.
• W3099681195 hasAuthorship W3099681195A5069079061 @default.
• W3099681195 hasAuthorship W3099681195A5085223431 @default.
• W3099681195 hasBestOaLocation W30996811951 @default.
• W3099681195 hasConcept C110472602 @default.
• W3099681195 hasConcept C121332964 @default.
• W3099681195 hasConcept C125857072 @default.
• W3099681195 hasConcept C1276947 @default.
• W3099681195 hasConcept C132552067 @default.
• W3099681195 hasConcept C150846664 @default.
• W3099681195 hasConcept C168589115 @default.
• W3099681195 hasConcept C170886286 @default.
• W3099681195 hasConcept C189159749 @default.
• W3099681195 hasConcept C44870925 @default.
• W3099681195 hasConcept C5788528 @default.
• W3099681195 hasConcept C98176478 @default.
• W3099681195 hasConceptScore W3099681195C110472602 @default.
• W3099681195 hasConceptScore W3099681195C121332964 @default.
• W3099681195 hasConceptScore W3099681195C125857072 @default.
• W3099681195 hasConceptScore W3099681195C1276947 @default.
• W3099681195 hasConceptScore W3099681195C132552067 @default.
• W3099681195 hasConceptScore W3099681195C150846664 @default.
• W3099681195 hasConceptScore W3099681195C168589115 @default.
• W3099681195 hasConceptScore W3099681195C170886286 @default.
• W3099681195 hasConceptScore W3099681195C189159749 @default.
• W3099681195 hasConceptScore W3099681195C44870925 @default.
• W3099681195 hasConceptScore W3099681195C5788528 @default.
• W3099681195 hasConceptScore W3099681195C98176478 @default.
• W3099681195 hasIssue "2" @default.
• W3099681195 hasLocation W30996811951 @default.
• W3099681195 hasLocation W30996811952 @default.
• W3099681195 hasOpenAccess W3099681195 @default.
• W3099681195 hasPrimaryLocation W30996811951 @default.
• W3099681195 hasRelatedWork W1502923089 @default.
• W3099681195 hasRelatedWork W1618018936 @default.
• W3099681195 hasRelatedWork W2007219364 @default.
• W3099681195 hasRelatedWork W2023725166 @default.
• W3099681195 hasRelatedWork W2109003336 @default.

• next