Directly to content
  1. Publishing |
  2. Search |
  3. Browse |
  4. Recent items rss |
  5. Open Access |
  6. Jur. Issues |
  7. DeutschClear Cookie - decide language by browser settings

Galaxy Shapes through Cosmic Time : Intrinsic Structure of Early-type Galaxies at High Redshift

Chang, Yu-Yen

PDF, English
Download (10MB) | Terms of use

Citation of documents: Please do not cite the URL that is displayed in your browser location input, instead use the persistent URL or the URN below, as we can guarantee their long-time accessibility.


In this thesis, we measure for the first time the projected shapes of large samples of distant early-type galaxies in deep near-infrared surveys from the ground and with the Hubble Space Telescope, and reconstruct their intrinsic, three-dimensional shape distribution assuming random viewing angles. We find that the most massive early-type galaxies are roundest at all redshifts 0 < z < 2.5, indicating that at any cosmic time mergers dominate the growth of the most massive galaxies. However, early-type galaxies were on average more disk-like at earlier times, indicating that star formation in their progenitors occurred in disks, and that merging is the dominant evolutionary channel after star formation ceases. Together with the recent finding that typical early-type galaxy sizes increase dramatically between z ~ 2 and the present, the increased `roundness' suggests that classical elliptical galaxies emerge through gradual merging and accretion of satellites. Moreover, the observed increase in number density over the same time span suggests that new early-type galaxies form continuously, also at late cosmic times. Our findings suggest that these newly formed early types are generally disk-like at all redshifts, and subsequently become larger and rounder through merging. In addition, we provide a low-redshift benchmark for high-redshift galaxy studies, by deriving new stellar mass and star formation rate estimates for nearly a million galaxies drawn from Sloan Digital Sky Survey spectroscopic sample. Our novel approach combines photometry from multiple surveys that span a large range in wavelength (from 0.4 to 22 micron), and uses the latest modeling techniques to consistently incorporate the effects of extinction and emission by dust. We use these new properties to investigate the nature of the bimodality of star formation activity in the galaxy population.

Item Type: Dissertation
Supervisor: Rix, Prof. Dr. Hans-Walter
Date of thesis defense: 17 December 2013
Date Deposited: 13 Jan 2014 12:33
Date: 2013
Faculties / Institutes: The Faculty of Physics and Astronomy > Dekanat der Fakultät für Physik und Astronomie
Subjects: 520 Astronomy and allied sciences
About | FAQ | Contact | Imprint |
OA-LogoDINI certificate 2013Logo der Open-Archives-Initiative