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  • Oxford University Press (OUP)  (1)
  • English  (1)
  • 2000-2004  (1)
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  • Oxford University Press (OUP)  (1)
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  • English  (1)
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    Online Resource
    Online Resource
    Bulge Formation in Late-Type Galaxies—Cuspy–vs Soft-Core Dark-Matter Density Profiles
    Oxford University Press (OUP) ; 2003
    In:  Publications of the Astronomical Society of Japan Vol. 55, No. 6 ( 2003-12-25), p. L89-L93
    Details
    In: Publications of the Astronomical Society of Japan, Oxford University Press (OUP), Vol. 55, No. 6 ( 2003-12-25), p. L89-L93
    Abstract: The dynamical evolution of super star clusters has been investigated in dark-matter halos depicted with a cuspy- or soft-core density profile. Simulations show that (1) exponential bulges with central cusps form in both cases; (2) distinctive bulge formation fractions are derived for cuspy- and soft-core profiles; (3) the masses of the formed bulges are causally connected with the masses of nuclear clusters, which are heavier in the case of a cuspy-core profile; (4) massive, nuclear star clusters possibly form with no discernible bulges at different ages in cuspy- or soft-core cases. Based on comparisons with observations, both the soft- and cuspy-core dark matter density profiles are suitable to relevant dwarf galaxies.
    Type of Medium: Online Resource
    ISSN: 0004-6264 , 2053-051X
    URL: Article
    DOI: 10.1093/pasj/55.6.L89
    RVK:
    US 1090
    Language: English
    Publisher: Oxford University Press (OUP)
    Publication Date: 2003
    detail.hit.zdb_id: 2206640-8
    detail.hit.zdb_id: 2083084-1
    SSG: 16,12
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