Matches in SemOpenAlex for { <https://semopenalex.org/work/W3128304004> ?p ?o ?g. }
- W3128304004 endingPage "2" @default.
- W3128304004 startingPage "2" @default.
- W3128304004 abstract "Young massive clusters (YMCs) are dense aggregates of young stars, which are essential to galaxy evolution, owing to their ultraviolet radiation, stellar winds, and supernovae. The typical mass and radius of YMCs are M ∼ 104 M⊙ and R ∼ 1 pc, respectively, indicating that many stars are located in a small region. The formation of YMC precursor clouds may be difficult because a very compact massive cloud should be formed before stellar feedback blows off the cloud. Recent observational studies suggest that YMCs can be formed as a consequence of the fast H i gas collision with a velocity of ∼100 km s−1, which is the typical velocity of the galaxy–galaxy interaction. In this study, we examine whether the fast H i gas collision triggers YMC formation using three-dimensional magnetohydrodynamics simulations, which includes the effects of self-gravity, radiative cooling/heating, and chemistry. We demonstrate that massive gravitationally bound gas clumps with M > 104 M⊙ and L ∼ 4 pc are formed in the shock compressed region induced by the fast H i gas collision, in which massive gas clumps can evolve into YMCs. Our results show that the YMC precursors are formed by the global gravitational collapse of molecular clouds, and YMCs can be formed even in low-metal environments, such as the Magellanic Clouds. Additionally, the very massive YMC precursor cloud, with M > 105 M⊙, can be created when we consider the fast collision of H i clouds, which may explain the origin of the very massive stellar cluster R136 system in the Large Magellanic Cloud." @default.
- W3128304004 created "2021-02-15" @default.
- W3128304004 creator A5049228892 @default.
- W3128304004 creator A5070168437 @default.
- W3128304004 creator A5085873695 @default.
- W3128304004 date "2021-02-08" @default.
- W3128304004 modified "2023-10-14" @default.
- W3128304004 title "Formation of Massive Star Clusters by Fast H i Gas Collision" @default.
- W3128304004 cites W1933730128 @default.
- W3128304004 cites W1966247736 @default.
- W3128304004 cites W1966842402 @default.
- W3128304004 cites W1968137411 @default.
- W3128304004 cites W1977521416 @default.
- W3128304004 cites W1979348280 @default.
- W3128304004 cites W1979773910 @default.
- W3128304004 cites W1993230081 @default.
- W3128304004 cites W1993244035 @default.
- W3128304004 cites W1994043374 @default.
- W3128304004 cites W1994064878 @default.
- W3128304004 cites W1995016890 @default.
- W3128304004 cites W2004052728 @default.
- W3128304004 cites W2004441263 @default.
- W3128304004 cites W2004549309 @default.
- W3128304004 cites W2004597566 @default.
- W3128304004 cites W2007156045 @default.
- W3128304004 cites W2007687569 @default.
- W3128304004 cites W2012952401 @default.
- W3128304004 cites W2014904361 @default.
- W3128304004 cites W2019532856 @default.
- W3128304004 cites W2026328109 @default.
- W3128304004 cites W2030159020 @default.
- W3128304004 cites W2037809736 @default.
- W3128304004 cites W2051468747 @default.
- W3128304004 cites W2053289371 @default.
- W3128304004 cites W2058373358 @default.
- W3128304004 cites W2061435934 @default.
- W3128304004 cites W2062671361 @default.
- W3128304004 cites W2062881881 @default.
- W3128304004 cites W2069333643 @default.
- W3128304004 cites W2069719190 @default.
- W3128304004 cites W2073147034 @default.
- W3128304004 cites W2078001023 @default.
- W3128304004 cites W2085514986 @default.
- W3128304004 cites W2085631143 @default.
- W3128304004 cites W2108751611 @default.
- W3128304004 cites W2119285898 @default.
- W3128304004 cites W2123177123 @default.
- W3128304004 cites W2127476512 @default.
- W3128304004 cites W2140888726 @default.
- W3128304004 cites W2242733211 @default.
- W3128304004 cites W2546954148 @default.
- W3128304004 cites W2568253711 @default.
- W3128304004 cites W2597663961 @default.
- W3128304004 cites W2760851005 @default.
- W3128304004 cites W2925297590 @default.
- W3128304004 cites W2963105353 @default.
- W3128304004 cites W2963786164 @default.
- W3128304004 cites W2990814396 @default.
- W3128304004 cites W3013571233 @default.
- W3128304004 cites W3014096975 @default.
- W3128304004 cites W3023099154 @default.
- W3128304004 cites W3098131598 @default.
- W3128304004 cites W3098252667 @default.
- W3128304004 cites W3098534401 @default.
- W3128304004 cites W3098814682 @default.
- W3128304004 cites W3099066325 @default.
- W3128304004 cites W3099100045 @default.
- W3128304004 cites W3099770833 @default.
- W3128304004 cites W3099915657 @default.
- W3128304004 cites W3100488602 @default.
- W3128304004 cites W3100648229 @default.
- W3128304004 cites W3101037996 @default.
- W3128304004 cites W3101601193 @default.
- W3128304004 cites W3101647161 @default.
- W3128304004 cites W3101764701 @default.
- W3128304004 cites W3102353139 @default.
- W3128304004 cites W3103692774 @default.
- W3128304004 cites W3103875916 @default.
- W3128304004 cites W3104713475 @default.
- W3128304004 cites W3105884397 @default.
- W3128304004 cites W3106325833 @default.
- W3128304004 cites W3106346103 @default.
- W3128304004 cites W3121654340 @default.
- W3128304004 cites W3121954543 @default.
- W3128304004 cites W3122777518 @default.
- W3128304004 cites W3124281809 @default.
- W3128304004 cites W3125933144 @default.
- W3128304004 cites W638594347 @default.
- W3128304004 doi "https://doi.org/10.3847/1538-4357/abcc75" @default.
- W3128304004 hasPublicationYear "2021" @default.
- W3128304004 type Work @default.
- W3128304004 sameAs 3128304004 @default.
- W3128304004 citedByCount "8" @default.
- W3128304004 countsByYear W31283040042021 @default.
- W3128304004 countsByYear W31283040042022 @default.
- W3128304004 countsByYear W31283040042023 @default.
- W3128304004 crossrefType "journal-article" @default.
- W3128304004 hasAuthorship W3128304004A5049228892 @default.