Matches in SemOpenAlex for { <https://semopenalex.org/work/W2008494046> ?p ?o ?g. }
- W2008494046 endingPage "L40" @default.
- W2008494046 startingPage "L36" @default.
- W2008494046 abstract "We examine whether the super star-forming clumps (R~1-3 kpc; M~10^8-10^9.5 Msun) now known to be a key component of star-forming galaxies at z~2 could be the formation sites of the locally observed old globular cluster population. We find that the stellar populations of these super star-forming clumps are excellent matches to those of local metal-rich globular clusters. Moreover, this globular cluster population is known to be associated with the bulges / thick disks of galaxies, and we show that its spatial distribution and kinematics are consistent with the current understanding of the assembly of bulges and thick disks from super star-forming clumps at high redshift. Finally, with the assumption that star formation in these clumps proceeds as a scaled-up version of local star formation in molecular clouds, this formation scenario reproduces the observed numbers and mass spectra of metal-rich globular clusters. The resulting link between the turbulent and clumpy disks observed in high-redshift galaxies and a local globular cluster population provides a plausible co-evolutionary scenario for several of the major components of a galaxy: the bulge, the thick disk, and one of the globular cluster populations." @default.
- W2008494046 created "2016-06-24" @default.
- W2008494046 creator A5027557571 @default.
- W2008494046 creator A5032049136 @default.
- W2008494046 creator A5091386388 @default.
- W2008494046 date "2010-03-21" @default.
- W2008494046 modified "2023-10-16" @default.
- W2008494046 title "Star-forming galaxies atz∼ 2 and the formation of the metal-rich globular cluster population" @default.
- W2008494046 cites W1524092957 @default.
- W2008494046 cites W1972341431 @default.
- W2008494046 cites W1972443998 @default.
- W2008494046 cites W1973331810 @default.
- W2008494046 cites W1974665753 @default.
- W2008494046 cites W1980350013 @default.
- W2008494046 cites W1986486448 @default.
- W2008494046 cites W1989714007 @default.
- W2008494046 cites W1989824204 @default.
- W2008494046 cites W1990491187 @default.
- W2008494046 cites W1991052054 @default.
- W2008494046 cites W1993244035 @default.
- W2008494046 cites W1993642111 @default.
- W2008494046 cites W1997384998 @default.
- W2008494046 cites W1998014385 @default.
- W2008494046 cites W2005638704 @default.
- W2008494046 cites W2005639341 @default.
- W2008494046 cites W2012983802 @default.
- W2008494046 cites W2013013065 @default.
- W2008494046 cites W2013575191 @default.
- W2008494046 cites W2020356115 @default.
- W2008494046 cites W2027091322 @default.
- W2008494046 cites W2035620374 @default.
- W2008494046 cites W2036949958 @default.
- W2008494046 cites W2037809736 @default.
- W2008494046 cites W2047172810 @default.
- W2008494046 cites W2048623741 @default.
- W2008494046 cites W2052014526 @default.
- W2008494046 cites W2066414969 @default.
- W2008494046 cites W2067239832 @default.
- W2008494046 cites W2073123016 @default.
- W2008494046 cites W2073236198 @default.
- W2008494046 cites W2077537026 @default.
- W2008494046 cites W2081243021 @default.
- W2008494046 cites W2081425105 @default.
- W2008494046 cites W2081705359 @default.
- W2008494046 cites W2082986345 @default.
- W2008494046 cites W2083761364 @default.
- W2008494046 cites W2085887670 @default.
- W2008494046 cites W2091617664 @default.
- W2008494046 cites W2093125763 @default.
- W2008494046 cites W2093395954 @default.
- W2008494046 cites W2094142432 @default.
- W2008494046 cites W2102825905 @default.
- W2008494046 cites W2109329782 @default.
- W2008494046 cites W2121665488 @default.
- W2008494046 cites W2123681429 @default.
- W2008494046 cites W2143468430 @default.
- W2008494046 cites W2144760780 @default.
- W2008494046 cites W2150995848 @default.
- W2008494046 cites W2163031519 @default.
- W2008494046 cites W2164574833 @default.
- W2008494046 cites W2599734048 @default.
- W2008494046 cites W3098183032 @default.
- W2008494046 cites W3098218686 @default.
- W2008494046 cites W3098387187 @default.
- W2008494046 cites W3098494936 @default.
- W2008494046 cites W3098683120 @default.
- W2008494046 cites W3100334553 @default.
- W2008494046 cites W3100401077 @default.
- W2008494046 cites W3100476555 @default.
- W2008494046 cites W3100568389 @default.
- W2008494046 cites W3102467437 @default.
- W2008494046 cites W3103833345 @default.
- W2008494046 cites W3104164168 @default.
- W2008494046 cites W3105652124 @default.
- W2008494046 cites W3123720894 @default.
- W2008494046 cites W3126143209 @default.
- W2008494046 doi "https://doi.org/10.1111/j.1745-3933.2010.00810.x" @default.
- W2008494046 hasPublicationYear "2010" @default.
- W2008494046 type Work @default.
- W2008494046 sameAs 2008494046 @default.
- W2008494046 citedByCount "88" @default.
- W2008494046 countsByYear W20084940462012 @default.
- W2008494046 countsByYear W20084940462013 @default.
- W2008494046 countsByYear W20084940462014 @default.
- W2008494046 countsByYear W20084940462015 @default.
- W2008494046 countsByYear W20084940462016 @default.
- W2008494046 countsByYear W20084940462017 @default.
- W2008494046 countsByYear W20084940462018 @default.
- W2008494046 countsByYear W20084940462019 @default.
- W2008494046 countsByYear W20084940462020 @default.
- W2008494046 countsByYear W20084940462021 @default.
- W2008494046 countsByYear W20084940462022 @default.
- W2008494046 countsByYear W20084940462023 @default.
- W2008494046 crossrefType "journal-article" @default.
- W2008494046 hasAuthorship W2008494046A5027557571 @default.
- W2008494046 hasAuthorship W2008494046A5032049136 @default.
- W2008494046 hasAuthorship W2008494046A5091386388 @default.
- W2008494046 hasBestOaLocation W20084940461 @default.