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- W3105191946 endingPage "L24" @default.
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- W3105191946 abstract "Recent deep Hubble Space Telescope WFC3 imaging suggests that a majority of compact quiescent massive galaxies at z~2 may contain disks. To investigate this claim, we have compared the ellipticity distribution of 31 carefully selected high-redshift massive quiescent compact galaxies to a set of mass-selected ellipticity and Sersic index distributions obtained from 2D structural fits to ~40,000$ nearby galaxies from the Sloan Digital Sky Survey. A Kolmogorov-Smirnov test shows that the distribution of ellipticities for the high-redshift galaxies is consistent with the ellipticity distribution of a similarly chosen sample of massive early-type galaxies. However the distribution of Sersic indices for the high-redshift sample is inconsistent with that of local early-type galaxies, and instead resembles that of local disk-dominated populations. The mismatch between the properties of high-redshift compact galaxies and those of both local early-type and disk-dominated systems leads us to conclude that the basic structures of high-redshift compact galaxies probably do not closely resemble those of any single local galaxy population. Any galaxy population analog to the high-redshift compact galaxies that exists at the current epoch is either a mix of different types of galaxies, or possibly a unique class of objects on their own." @default.
- W3105191946 created "2020-11-23" @default.
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- W3105191946 date "2012-07-12" @default.
- W3105191946 modified "2023-10-13" @default.
- W3105191946 title "ON THE SHAPES AND STRUCTURES OF HIGH-REDSHIFT COMPACT GALAXIES" @default.
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- W3105191946 doi "https://doi.org/10.1088/2041-8205/754/2/l24" @default.
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