FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2596602655> ?p ?o ?g. }

• W2596602655 abstract "Rotation plays a key role in the star-formation process, from pre-stellar cores to pre-main-sequence (PMS) objects. Understanding the formation of massive stars requires taking into account the accretion of angular momentum during their PMS phase. We study the PMS evolution of objects destined to become massive stars by accretion, focusing on the links between the physical conditions of the environment and the rotational properties of young stars. In particular, we look at the physical conditions that allow the production of massive stars by accretion. We present PMS models computed with a new version of the Geneva Stellar Evolution code self-consistently including accretion and rotation according to various accretion scenarios for mass and angular momentum. We describe the internal distribution of angular momentum in PMS stars accreting at high rates and we show how the various physical conditions impact their internal structures, evolutionary tracks, and rotation velocities during the PMS and the early main sequence. We find that the smooth angular momentum accretion considered in previous studies leads to an angular momentum barrier and does not allow the formation of massive stars by accretion. A braking mechanism is needed in order to circumvent this angular momentum barrier. This mechanism has to be efficient enough to remove more than 2/3 of the angular momentum from the inner accretion disc. Due to the weak efficiency of angular momentum transport by shear instability and meridional circulation during the accretion phase, the internal rotation profiles of accreting stars reflect essentially the angular momentum accretion history. As a consequence, careful choice of the angular momentum accretion history allows circumvention of any limitation in mass and velocity, and production of stars of any mass and velocity compatible with structure equations." @default.
• W2596602655 created "2017-03-23" @default.
• W2596602655 creator A5006202137 @default.
• W2596602655 creator A5008797753 @default.
• W2596602655 creator A5039093383 @default.
• W2596602655 creator A5056081506 @default.
• W2596602655 creator A5061920593 @default.
• W2596602655 creator A5062809181 @default.
• W2596602655 date "2017-03-24" @default.
• W2596602655 modified "2023-09-25" @default.
• W2596602655 title "Massive star formation by accretion II. Rotation: how to circumvent the angular momentum barrier?" @default.
• W2596602655 cites W1564894563 @default.
• W2596602655 cites W1868137405 @default.
• W2596602655 cites W1959491247 @default.
• W2596602655 cites W1976565017 @default.
• W2596602655 cites W1978253505 @default.
• W2596602655 cites W1978391636 @default.
• W2596602655 cites W1979896981 @default.
• W2596602655 cites W1986652040 @default.
• W2596602655 cites W1995295165 @default.
• W2596602655 cites W2006124034 @default.
• W2596602655 cites W2007219364 @default.
• W2596602655 cites W2012799415 @default.
• W2596602655 cites W2016893051 @default.
• W2596602655 cites W2024256120 @default.
• W2596602655 cites W2035591344 @default.
• W2596602655 cites W2041629736 @default.
• W2596602655 cites W2046756693 @default.
• W2596602655 cites W2054419610 @default.
• W2596602655 cites W2057253091 @default.
• W2596602655 cites W2065925884 @default.
• W2596602655 cites W2065979430 @default.
• W2596602655 cites W2069001906 @default.
• W2596602655 cites W2080628829 @default.
• W2596602655 cites W2082250392 @default.
• W2596602655 cites W2095668713 @default.
• W2596602655 cites W2114574183 @default.
• W2596602655 cites W2129495060 @default.
• W2596602655 cites W2134992552 @default.
• W2596602655 cites W2137848797 @default.
• W2596602655 cites W2139243881 @default.
• W2596602655 cites W2141687171 @default.
• W2596602655 cites W2143517154 @default.
• W2596602655 cites W2144976183 @default.
• W2596602655 cites W2152832294 @default.
• W2596602655 cites W2153169334 @default.
• W2596602655 cites W2159730530 @default.
• W2596602655 cites W2161278663 @default.
• W2596602655 cites W2295206435 @default.
• W2596602655 cites W2347347915 @default.
• W2596602655 cites W2486386552 @default.
• W2596602655 cites W2515384401 @default.
• W2596602655 cites W2540128138 @default.
• W2596602655 cites W3101118831 @default.
• W2596602655 cites W3102037608 @default.
• W2596602655 cites W3105393663 @default.
• W2596602655 cites W3106258018 @default.
• W2596602655 cites W3124221894 @default.
• W2596602655 cites W3207945521 @default.
• W2596602655 cites W3216097261 @default.
• W2596602655 hasPublicationYear "2017" @default.
• W2596602655 type Work @default.
• W2596602655 sameAs 2596602655 @default.
• W2596602655 citedByCount "0" @default.
• W2596602655 crossrefType "journal-article" @default.
• W2596602655 hasAuthorship W2596602655A5006202137 @default.
• W2596602655 hasAuthorship W2596602655A5008797753 @default.
• W2596602655 hasAuthorship W2596602655A5039093383 @default.
• W2596602655 hasAuthorship W2596602655A5056081506 @default.
• W2596602655 hasAuthorship W2596602655A5061920593 @default.
• W2596602655 hasAuthorship W2596602655A5062809181 @default.
• W2596602655 hasConcept C110472602 @default.
• W2596602655 hasConcept C121332964 @default.
• W2596602655 hasConcept C1276947 @default.
• W2596602655 hasConcept C150846664 @default.
• W2596602655 hasConcept C155675718 @default.
• W2596602655 hasConcept C20782240 @default.
• W2596602655 hasConcept C2776401274 @default.
• W2596602655 hasConcept C44870925 @default.
• W2596602655 hasConcept C45193367 @default.
• W2596602655 hasConcept C56181872 @default.
• W2596602655 hasConcept C74650414 @default.
• W2596602655 hasConceptScore W2596602655C110472602 @default.
• W2596602655 hasConceptScore W2596602655C121332964 @default.
• W2596602655 hasConceptScore W2596602655C1276947 @default.
• W2596602655 hasConceptScore W2596602655C150846664 @default.
• W2596602655 hasConceptScore W2596602655C155675718 @default.
• W2596602655 hasConceptScore W2596602655C20782240 @default.
• W2596602655 hasConceptScore W2596602655C2776401274 @default.
• W2596602655 hasConceptScore W2596602655C44870925 @default.
• W2596602655 hasConceptScore W2596602655C45193367 @default.
• W2596602655 hasConceptScore W2596602655C56181872 @default.
• W2596602655 hasConceptScore W2596602655C74650414 @default.
• W2596602655 hasOpenAccess W2596602655 @default.
• W2596602655 hasRelatedWork W1571085112 @default.
• W2596602655 hasRelatedWork W1626127214 @default.
• W2596602655 hasRelatedWork W1761901654 @default.
• W2596602655 hasRelatedWork W1982357974 @default.
• W2596602655 hasRelatedWork W1989357618 @default.
• W2596602655 hasRelatedWork W1989635374 @default.

• next